The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central bulge that appears largely spheroidal, with a gradual decrease in luminosity extending outwards. There is only a suggestion of a disk-like structure and no distinct spiral arms are evident. The color profile of the galaxy indicates a predominantly older stellar population; the central bulge emits a yellowish-white light, shifting to slightly redder tones in the outer regions. There are no obvious signs of ongoing major mergers or significant tidal disturbances. Overall, the galaxy has the characteristics of an elliptical or possibly an early-type spiral galaxy with minimal star formation.
