The galaxy presents an elliptical morphology, appearing largely smooth and concentrated. The light distribution is centrally concentrated with a bright core, gradually diminishing outward. There are no visually apparent spiral arms or prominent dust lanes. The color appears relatively uniform across the galaxy, shifting from yellow in the core to a bluish-white tinge toward the outer edges of the ellipse, potentially indicating older stellar populations dominating the center, with a small amount of new stars formed around the outer edges of the galaxy. The isophotes seem generally smooth and well-defined, showing no apparent major distortions indicating recent major merger events, though there might be minor irregularities suggesting past interactions or internal dynamics at play.
