The galaxy presents a generally smooth morphology, with a concentration of light towards the center, suggesting a prominent bulge. The object displays a slight ellipticity; it is neither perfectly spherical nor highly elongated. There is no clear indication of spiral arm structure or significant dust lanes within the galaxy. Color gradients are subtle, with the central region appearing more yellow/orange, possibly indicating an older stellar population. The outer regions appear slightly bluer, hinting at the presence of some younger stars or ongoing star formation, albeit at a low rate. No obvious signs of major merger activity, such as tidal tails or strong distortions, are apparent, though a slight asymmetry might indicate a minor past interaction or internal disturbance.
