The galaxy appears to be a relatively smooth, elliptical system with a notable elongation. It exhibits a central concentration of light that fades gradually outward. The core region presents a yellowish hue, potentially indicating an older stellar population dominating the center. Fainter, bluer light surrounds the central region, possibly suggesting some ongoing star formation or a younger stellar component in the outer regions. There are hints of minor asymmetries or disturbances in the outer halo, although overall the galaxy appears relatively undisturbed. The general form is an elliptical shape, rather than a spiral.
