The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated light profile. Its color suggests an older stellar population. The central region appears brighter than the surrounding halo, indicative of a concentration of stars towards the galactic nucleus. There is no evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, without obvious signs of ongoing mergers or tidal interactions. Its overall appearance suggests a system that has largely completed its star formation. The slight ellipticity suggests some rotational support, although not dominating the overall morphology. The galaxy is relatively compact.