The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile suggests a dominant population of older stars, as indicated by the yellowish-red hue of the galactic center. The overall structure appears undisturbed, showing no obvious signs of tidal interactions or major mergers. There may be limited star formation occuring. The galaxy appears to be relatively symmetrical in shape, with a slight deviation from perfect circularity.
