The galaxy presents as a fairly smooth, elliptical-like structure. It has a concentrated central bulge, which transitions into a more diffuse halo region. There is a noticeable color gradient from the center outwards; the central region appears more yellowish or orange, suggesting an older stellar population. The outer regions exhibit slightly bluer hues indicating the presence of some younger stars or star-forming regions, though the overall star formation rate seems relatively low. The overall shape appears mostly round, lacking any strong indications of spiral arms or a bar structure. There are no obvious signs of any major mergers or tidal disturbances, although there might be a slight asymmetry suggesting a minor past interaction.
