You might be thinking of the Hubble Ultra Deep Field image (
https://science.nasa.gov/asset/hubble/hubble-ultra-deep-fiel...). I believe it was the result of NASA saying "Let's look at what appears to be a completely dark spot in space, zoom in as far as we can, and see what's there."
We see stars in our galaxy because they are close enough to us that we see them as individual stars. Compare that to the Andromeda Galaxy, which is far enough away that without intense zoom, it looks like a single source of light. There are galaxies even farther away, which we cannot see with the naked eye at all, but zooming in on them like Hubble did means we eventually get enough resolution to see they are individual galaxies, unfathomably far away.
JWST being able to see infrared means we'll see galaxies that are so far away, their light is redshifted so we (and Hubble) cannot even see them at all.
With regards to your question about how to test the bubble hypothesis posted by parent, we would be limited by how variable our point of view can be. We can gather what data we can at one end of Earth's orbit, and then try to see from the opposite end and compare what we see, comparing data sets to see if certain galaxies or stars are in different positions. We already do some of this when dealing with gravitational lensing and I believe it's one of the primary ways we can detect black holes, as they bend light a lot.