The galaxy presents as a relatively compact, elliptical-like structure. Its central region displays a bright, concentrated core, suggesting a significant concentration of stars. The light appears fairly smooth, without any obvious substructure or spiral arms. The galaxy exhibits a fuzzy, diffuse halo extending outward from the core, with the color becoming slightly bluer towards the outer edges, potentially indicating younger stellar populations in these regions. The galaxy has a shape that is something in between round and elongated. Overall, the galaxy seems to be relatively isolated, without any obvious signs of major interactions. There may be some minor disturbances.
