The galaxy presents as a smooth, elliptical structure, elongated slightly along its major axis. It exhibits a high degree of central concentration, with a bright, yellowish core that gradually fades into a more diffuse halo. There is no evidence of spiral arms or significant dust lanes. The overall color suggests a population of older stars with relatively low ongoing star formation. The galaxy appears undisturbed, without any signs of tidal tails, mergers, or significant morphological disturbances. Based on its shape and color, it likely represents a massive galaxy toward the high end of the mass spectrum.
