The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with a slight elongation that might indicate a mild deviation from perfect sphericity. There is a distinct color gradient from the center outwards, with the core region displaying a more yellow-orange hue, which suggests a population of older stars. The outer regions appear somewhat bluer, potentially indicating the presence of younger stars. The galaxy lacks any prominent spiral arm structure or strong dust lanes. There is potentially evidence of a minor interaction, as indicated by the slight asymmetry on the south side of the core.
