The galaxy appears to be a relatively smooth, elliptical-type galaxy with a slight degree of elongation. It exhibits a concentrated central bulge and a gradual decrease in luminosity towards its outer edges. The color is generally yellow, suggesting an older stellar population with lower levels of ongoing star formation. There is a possible minor disturbance or slight asymmetry visible in the morphology, but the galaxy is not undergoing a major merger. The overall structure indicates a well-established and relatively undisturbed system.
