The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light profile. It exhibits a yellowish-white hue, suggesting a stellar population dominated by older, evolved stars. The galaxy is nearly circular in appearance, with a slight elongation. No distinct spiral arm structures or dust lanes are visible. There is a gradual decrease in surface brightness from the core to the outer regions, further reinforcing its classification as an elliptical galaxy. The absence of prominent features indicates a relatively quiescent system, with little ongoing star formation.
