The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions gradually into a more diffuse halo. There is a slight elongation apparent. The primary color gradient shifts from a yellowish-orange hue in the core region to a greenish color in the outer parts of the galaxy. No apparent spiral arm structures or dust lanes are visible. There does not appear to be any evidence of ongoing or recent major merger activity, though a possible slight disturbance can not be fully ruled out. The galaxy appears relatively isolated within the field.
