This galaxy appears to be a relatively smooth, elliptical or lenticular system. The light distribution is concentrated towards the center, with a clear bulge component that is yellowish in color. The outer regions of the galaxy display a bluer hue, possibly indicating the presence of a younger stellar population compared to the core. The overall shape is elongated, but not highly flattened, suggesting it is not a spiral galaxy. There is no obvious presence of spiral arms or significant dust lanes. No signs of tidal disturbances or ongoing mergers with other galaxies are visibly present, which suggests that it is an isolated system that has been undisturbed for some time.
