The galaxy presents an elliptical morphology, appearing relatively smooth and concentrated. The central region exhibits a high degree of brightness, suggesting a significant concentration of stars or an active galactic nucleus. A slight extension or possible tidal feature is observed on one side, indicating a potential minor interaction or disturbance. The galaxy displays a gradient in color, with the central core exhibiting a bluer hue, possibly indicative of younger stellar populations. The outer regions appear redder, suggesting older, cooler stars. There is no clear evidence of spiral arm structures or a distinct disk.