This galaxy exhibits a flattened, elliptical morphology, appearing intermediate in shape between round and elongated. The primary light distribution is smooth and centrally concentrated, transitioning to a fainter, more diffuse halo or outskirts. The color gradient suggests an aging stellar population, with a yellowish-orange hue dominating the central region and subtly bluer tones in the outer regions. Although appearing mostly undisturbed, there are subtle asymmetries in the outer regions that hint at minor gravitational interactions or past mergers. The galaxy is moderately massive, suggesting the presence of a significant population of older stars, and has moderate ongoing star formation.
