The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a centrally concentrated bulge, with a radial decrease in luminosity towards the outer regions. There is a subtle color gradient, with the core appearing more yellow/orange than the outer regions, suggestive of an older stellar population in the center. The lack of apparent spiral arms or dust lanes points to a classification as an elliptical or lenticular galaxy. There is very little indication of any merger events, it has a relatively undisturbed appearance. The galaxy is fairly compact.
