The galaxy presents as a fairly smooth, elliptical-like object. It exhibits a concentrated central region, potentially a bulge, that appears more luminous and yellowish-white in color. There is little evidence of spiral arms or a prominent disk structure. The galaxy's overall shape is generally rounded. The surrounding halo appears somewhat diffuse, with a gradual decrease in luminosity from the core outwards. There are no apparent signs of a major ongoing merger or significant tidal disturbances, however, the possibility of a minor interaction cannot be ruled out. The galaxy appears relatively isolated.
