The galaxy presents an elliptical morphology, appearing mostly smooth with a concentrated central bulge. The light distribution indicates a centrally dominant spheroid. The galaxy exhibits a color gradient, with the core region appearing more yellow/gold, potentially indicating an older stellar population. There is a subtle color shift towards redder hues at the outer edges of the galaxy, again, suggesting possibly older stars within the extended halo. No distinct spiral arms or dust lanes are visible. The overall appearance suggests a relatively evolved system, consistent with a likely low star formation rate. There is no obvious evidence of any ongoing major mergers or strong tidal disturbances in this image.
