The galaxy presents as a smooth, elliptical structure with a bright, concentrated core. It exhibits a slight elongation, and its overall color appears to be dominated by a bluish-white hue. This bluer color suggests the presence of a younger stellar population within the galaxy. There are indications of some minor disturbances or asymmetries in its outer regions, suggesting possible interactions. The light distribution gradually fades from the bright center, conforming to an inner region that transitions smoothly into a more diffuse outer halo. The light concentration toward the center implies a high Sersic index, further pointing toward an elliptical galaxy morphology.
