The galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population. The light gradually diminishes outward, transitioning to a more diffuse, bluish-white color in the surrounding halo. This suggests the presence of a younger stellar population and ongoing, albeit potentially low-level, star formation activity in the outer regions. The overall form appears relatively undisturbed, with no obvious signs of major mergers or significant tidal disruptions. Slight asymmetries in the outer halo might indicate minor gravitational interactions with smaller satellite galaxies. The galaxy appears to be relatively smooth in texture.
