The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated, bright luminosity that gradually diminishes outward. The overall shape is somewhat rounded, though it appears slightly elongated along one axis. Faint, diffuse features suggest a possible, very subtle disk-like component. There is no strong evidence of spiral arms or prominent dust lanes. Additionally, a slight degree of asymmetry may be apparent, hinting at a possible past interaction or minor disturbance. It does not seem to have a major merger.
