The galaxy presents as a fairly smooth, elliptical-like structure. Its light profile indicates a concentrated central bulge with a gradual decrease in luminosity outwards, lacking discernible spiral arms or a well-defined disk. The galaxy exhibits a color gradient, appearing more yellow/orange towards the center, possibly indicating an older stellar population dominating the core with a lack of active star formation. The outer regions appear slightly bluer, suggesting the presence of younger stars or lower metallicity. There are no obvious signs of tidal disturbances or interactions with other galaxies, although the resolution is insufficient to rule out minor past mergers. It seems to be a relatively isolated system.
