The galaxy presents as a somewhat smooth, elliptical-like structure. It exhibits a central bulge that appears relatively bright and concentrated. The surrounding halo gradually fades outwards, displaying a more diffuse light distribution. There are subtle indications of a disk component or faint spiral arms, although they are not sharply defined. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal disruptions. The color profile suggests the presence of a mix of stellar populations, with a tendency towards older, redder stars in the central regions.
