The galaxy presents as an elliptical or lenticular system, exhibiting a smooth and largely featureless morphology. The light profile is centrally concentrated, with a noticeable decrease in surface brightness radiating outwards from the core. There appears to be a distinct spheroidal bulge component dominating the overall structure. The color is notably red, suggesting a population of older stars and a paucity of ongoing star formation. There is no evidence of spiral arms, prominent dust lanes, or tidal features indicative of recent or ongoing mergers. The overall impression is that of a mature and quiescent galaxy.
