The galaxy appears as a relatively compact, elliptical structure. It exhibits a smooth, centrally concentrated luminosity profile. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region and slightly bluer tones extending towards the outer edges. There is no evidence of spiral arms or a prominent disk, implying a likely classification as an elliptical galaxy. The galaxy shows little indication of significant star formation activity, and its overall structure suggests it is a well-relaxed system. There is no obvious sign of interaction with any other galaxy.