The galaxy presents an elliptical morphology. The galaxy exhibits a smooth, centrally concentrated luminosity profile. The core region appears redder in color, suggesting an older stellar population. The outer regions show a transition towards a slightly bluer hue, potentially indicating more recent, albeit modest, star formation activity. The overall structure suggests a galaxy that is relatively undisturbed, with no obvious signs of major mergers or tidal features. There is a slight asymmetry, with a more extended feature on one side. The galaxy has an apparent axis ratio that is not perfectly circular, displaying some degree of flattening.
