Strong gravitational lensing produces multiple images if the object lens and observer are in a specific alignment. This is due to there being multiple stationary points in the time arrival surface for the paths the light can take. So far I understand that.
Now what is puzzling me for a while is what prevents a classical lens, for lack of better term, from displaying the same behaviour? Is it just a lack of scale? In gravitational lenses we are dealing with massive scales so the speed of light comes into play where as your run of the mill spy glass doesn't really care about that.
So I guess what I'm asking is if I had a galaxy sized massless glass lens would it look the same as a gravitational lens?