The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on. There is a prominent central bulge that appears relatively smooth and concentrated. The disk itself is thin and elongated, and it has a fairly smooth texture, with little visible substructure or spiral arm features. There is no significant dust lane apparent and no notable ongoing major merging events. Overall, it seems to be a relatively quiescent disk galaxy observed at a moderate cosmological distance.
