The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile indicates a bias towards redder hues, which may suggest an older stellar population, and less ongoing star formation. The object lacks any apparent spiral arm structures or prominent dust lanes, and exhibits a degree of roundness. There are no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity. Faint hints of blue indicate areas of star formation.
