The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated light profile with a bright, yellowish core that fades into a more diffuse halo. The galaxy's shape is generally round, with a slight elongation. No distinct spiral arms or bar structures are discernible. There are no obvious signs of recent major merger activity or significant tidal disturbances. Faint color variations are present, indicating varying stellar populations within the galaxy. The central region presents a warmer, yellowish hue suggestive of older stars, while the outer regions appear slightly bluer, which may indicate a younger stellar population or ongoing, albeit subdued, star formation. Overall, the galaxy presents a quiescent appearance.
