The galaxy exhibits a centrally concentrated morphology, appearing largely smooth and elliptical in shape. There is a distinct central bulge which dominates the light profile, surrounded by a more diffuse halo. A slight color gradient is observed, with the central region appearing more yellow-orange, suggesting an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of younger stars or ongoing, albeit low-level, star formation. No obvious spiral arms or significant dust lanes are discernible within the galaxy's structure. There are no clear signs of a recent major merger or tidal disruption. The galaxy seems to be relatively isolated.
