The galaxy presents a largely smooth morphology, suggestive of an elliptical classification. The central bulge exhibits a concentrated, bright yellow-white hue, indicative of an older stellar population likely dominated by red giant stars. Moving outward from the core, the galaxy diffuses into a less concentrated halo. The outer regions display a bluer tint, possibly indicating the presence of younger, hotter stars or ongoing star formation, albeit at a relatively low rate. There is no discernible spiral structure or prominent dust lanes. The overall shape appears close to round. There are no visible signs of a major merger or tidal disturbances. Minor asymmetries or irregularities are present, perhaps indicating the presence of a small companion or recent, minor interaction.