The galaxy presents as a single, relatively smooth object with a moderately concentrated light profile. It displays a slight ellipticity, appearing more elongated than perfectly circular. The light distribution indicates a bulge-dominated morphology, lacking any distinct spiral arm structures. The color gradient suggests a stellar population with intermediate ages. There is a suggestion of some activity, with color variations across the galaxy indicating areas of potential active star formation. The galaxy appears largely undisturbed, showing no clear signs of ongoing major mergers or tidal distortions. There may be a minor companion nearby, but it is difficult to make conclusions based on image resolution. 
