The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that appears yellowish-white, suggestive of an older stellar population. Moving outwards from the center, a bluer halo or disk is barely visible, indicating the presence of some younger, hotter stars, although these regions are faint. The overall morphology appears relatively undisturbed, although there may be some subtle signs of minor tidal features or asymmetries present upon closer inspection. It may be undergoing a minor merger with a smaller galaxy. The galaxy does not show a strong spiral arm structure.
