The galaxy appears as a fairly smooth, elliptical-like structure. It presents a concentrated central bulge with a gradual decrease in luminosity towards the outer regions, indicating a relatively well-defined spheroidal component. There is a slight elongation observed, deviating somewhat from a perfect spherical shape, suggesting it may be an E3-E5 galaxy on the Hubble sequence. The light distribution seems to be dominated by older stellar populations, as inferred from the yellowish-white color, which typically implies a paucity of ongoing star formation activity. Faint, diffuse outer regions extend beyond the main body, with a slight color variation from the center to the edges, where bluer hues become more prominent. I do not observe any signs of spiral arms or other distinct features indicating a disk, nor are there any signs of ongoing mergers or tidal disturbances.
