The galaxy presents as an elliptical or lenticular type, with a dominant smooth, centrally concentrated bulge. The galaxy exhibits a slightly elongated shape, leaning more towards round than cigar-shaped. The color profile suggests a population of older stars with a possible contribution from younger populations, indicated by the slight bluish tint in the outer regions. There is a noticeable lack of defined spiral arm structure or significant dust lanes. The morphology is largely undisturbed, with no evidence of major mergers or strong tidal interactions, though some minor disturbances cannot be ruled out. The overall impression is that of a relatively quiescent galaxy with ongoing, albeit low, star formation activity.
