The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be elliptical, with an aspect ratio that indicates a slight flattening. The radial light profile suggests a significant bulge component. The galaxy exhibits a color gradient, appearing more yellow-red in the central regions and slightly bluer towards the outer edges, possibly indicating older stellar populations concentrated towards the center. There is no obvious evidence of spiral arm structures or strong dust lanes. The overall color suggests it is likely an older galaxy with a relatively low rate of star formation. There are no obvious tidal features, suggesting it has not undergone a major merger recently.
