The galaxy presents a primarily smooth morphology, with a discernible central bulge region that appears significantly brighter and more concentrated than the outer regions. The overall shape of the galaxy is elliptical, exhibiting a moderate degree of ellipticity, not quite round, but also not particularly elongated. The color gradient suggests a population of older stars dominating the central bulge, appearing yellowish-white, while the outer regions show a hint of bluer tones, potentially indicating the presence of younger stellar populations and ongoing, albeit moderate, star formation activity. There is no apparent evidence of significant tidal disturbances or ongoing major merger activity based on the galaxy's structure, although a slight asymmetry might suggest a minor past interaction. The galaxy's relatively compact size and smooth features are consistent with a classification as an early-type spiral or lenticular galaxy at a considerable distance.
