The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its periphery. The color is primarily a yellowish hue, potentially indicating an older stellar population with lower ongoing star formation. The overall morphology suggests it is an early-type galaxy with no prominent spiral arms or significant dust lanes visible. There are potentially slight disturbances in the morphology which could mean past minor mergers. It has very rounded features.
