The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a relatively evolved stellar population. The galaxy appears mostly undisturbed, with no obvious signs of tidal features or major merger activity. The round shape and absence of spiral arms supports classification as an elliptical or S0 galaxy. The galaxy has an apparent yellow/orange hue, suggesting minimal ongoing star formation. The high mass likely indicates that this galaxy is in the more luminous range. The lack of any strong color gradients or distinct features indicates a relatively uniform composition and stellar density throughout.
