It would be interesting to model what sort of "zone" needs to exist, for galaxies to be close enough to overcome expansion, but far enough away not to crash into each other for however many zillions of years, such that we can witness it now
It would, but the calculation is intractable.
If we take a purely mathematical approach and try to model how three (or more) bodies of arbitrary mass, position, and momenta, would move at any given point... it turns out it's impossible. You simply cannot run through the algebra and say, "OK, if they had these initial conditions at
t = 0, they would have these conditions at
t =
t" - c'est impossiblé.
Instead, we have to use statistical approximation using iterations and computer simulations.
So, trying to model this galactic 'boundary' with so many variables would be
even more impossible (if that makes any sense

). You'd have to factor in your own galaxy's mass, the mass of the other galaxy, its position and velocity, etc,
and all the other factors like the other galaxies in the local area,
and you have to take into account the fact that galaxies aren't nice, discrete objects, but huge conglomerates of stars (the dynamics of stars within a galaxy is quite fascinating in itself).
And let's not even get started on dark matter...