The galaxy presents as an elliptical structure, with a high degree of central concentration. Its overall color suggests an older stellar population. There is a lack of well-defined spiral arms or significant dust lanes. The galaxy exhibits a smooth light profile, with a bright central bulge that appears slightly elongated. There's evidence of a more diffuse, fainter halo extending outward from the core, though it lacks pronounced features. A subtle color gradient is observed, with the central region appearing yellower than the outer regions, hinting at potential variations in stellar populations or metallicity within the galaxy.
