So if one were to take a pair of synchronized clocks and have them force each other apart so that they travel the same speed in either direction, then have the clocks stop when they reach a premeasured equal amount in both directions, could you compare the two stopped clock readings and determine if time dilation was anisotropic or isotropic, and therefore whether the speed of light was also anisotropic or isotropic?
No. Look at the Lorentz factor for flat 1+1-dimensional spacetime (e.g. that from special relativity):
$$\gamma(v)=\frac{1}{\sqrt{1-\frac{v^2}{c^2}}}.$$
Note that it is symmetric about the transformation $v\to -v$, so $\gamma(v)=\gamma(-v)$. Time dilation will necessarily be isotropic if special relativity is obeyed.
But wait, there might be a term in there linear in $v$ and which would break $v\to -v$ symmetry! Yes, you get this for example in the metric
$$ds^2=c^2dt^2-k^2dt^2-dx^2-2kdxdt.$$
In that case a term linear in $v$ does get added to the denominator in the Lorentz factor, arising directly from the $dxdt$ term in the line element. But of course, in these scenarios, you can coordinate-transform that term away. That line element is that of a coordinate system that has undergone a Galilean boost by $v_\text{boost}=k$, so of course anisotropy is introduced as a given, and you shouldn’t expect in this scenarios for ordinary SR’s isotropies to hold till you get back to a proper coordinate system.
There are situations where there is manifest curvature that produces off-diagonal terms above that can’t be whooshed away as easily. But in those cases, it only seems like the speed of light is anisotropic (or equivalently like two clocks would have different time dilation) if you try to check from a weird frame. Near a rotating black hole, off-diagonal terms appear as part of the Kerr metric, and won’t go away trivially, but the solution is to note that you are technically “physically rotating” around the black hole if you are not “coordinate-rotating” with it in the direction of rotation, insofar as for constant angular coordinates the metric near the BH looks exactly like one for a boosted coordinate system. So the proper thing to do is to boost into the frame where you are not physically rotating (ignoring the fact that you wouldn’t survive because in reality gravity would pull you in if you’re not orbiting), insodoing adding a rotation along with the black hole, and removing the terms that generate time dilation anisotropies.
All that is to say: the only scenario in GR where time dilation would be anisotropic is one where a simple Galilean boost (or Lorentzian if you prefer) removes the anisotropy.