The galaxy presents as a generally smooth and rounded object. It appears relatively featureless, lacking prominent spiral arms or a distinct bar structure. The color distribution is suggestive of an elliptical galaxy, with a concentrated, yellowish-white core indicative of an older stellar population. The outer regions exhibit a bluer hue, possibly indicating the presence of younger stars or ongoing, albeit subdued, star formation. There is a subtle suggestion of a disk-like component, though it is not sharply defined. No strong signs of a major merger or significant tidal disturbances are evident, though some minor asymmetry cannot be ruled out. Overall, the galaxy seems to be relatively evolved.
