The galaxy presents as a mostly smooth, elliptical-like structure. It exhibits a concentrated central bulge with a bright yellowish-white core, suggestive of an older stellar population. The outer regions of the galaxy appear more diffuse and are tinged with a greenish hue, possibly indicating the presence of some younger stars or ionized gas, though the overall star formation rate is likely low. The galaxy appears relatively undisturbed with no obvious signs of major mergers or significant tidal features. Its shape is slightly elongated but generally rounded. There may be minor asymmetries or subtle disturbances in the outer regions, but these are not prominent, and the galaxy appears to be relatively isolated.
