The galaxy presents as a smooth, elongated object. The light distribution suggests a centrally concentrated spheroid shape. A subtle color gradient is visible, with the core appearing slightly yellower compared to the bluer outer regions. There is little indication of spiral arm structure or significant dust lanes, suggesting a relatively undisturbed system. The overall morphology appears consistent with an elliptical galaxy, although the image resolution limits precise classification. The lack of any visible disruptions suggests a low probability of recent major merger events.
