The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. There is a decrease in luminosity radiating outward from the center. A slight asymmetry is observed in the outer regions suggesting a potential interaction or minor disturbance. The overall color appears yellowish, indicative of an older stellar population and potentially lower star formation rate, though some star formation is likely still present. The galaxy displays a round, not elongated appearance. There is no visible evidence of a significant merger.
