The galaxy presents as a relatively smooth object, with a high degree of central concentration. The light distribution indicates a spheroidal morphology. There is no obvious disk or spiral arm structure visible. The color gradient suggests a stellar population that is likely dominated by older stars, with perhaps a small amount of ongoing star formation or a younger population in the central region as indicated by the slightly bluer hue. No strong tidal features or signs of recent major merger events are apparent, although there may be some minor asymmetries in the outer isophotes hinting at minor interactions. The object appears to be relatively isolated within the field of view. The galaxy is nearly round in projection.
