The galaxy presents as a single, relatively smooth and centrally concentrated object. The main body exhibits a largely elliptical morphology, appearing quite round in overall shape. The luminosity profile indicates a substantial bulge component. The color appears yellow or orange, suggesting an older stellar population is dominant, with less active star formation currently occurring. A secondary, smaller, and dimmer object is located close to the galaxy on its periphery, possibly a smaller satellite galaxy or tidal remnant interacting with the primary galaxy. Overall, the galaxy appears relatively undisturbed, with no strong evidence of major mergers, though minor disturbances are possible.
