The galaxy presents a centrally concentrated morphology with a bright, yellowish core. The core region appears relatively smooth, lacking distinct features. Surrounding the core is a more diffuse, extended halo or bulge component, with a bluer hue, suggesting the presence of younger stellar populations than the central core. The overall shape appears somewhat elliptical, though there may be subtle indications of a faint disk structure oriented roughly horizontally. There are no clear signs of strong spiral arms or prominent dust lanes. The galaxy's outer regions fade gradually into the background sky. There may be evidence of minor disturbances or interactions, but the galaxy appears largely undisturbed.
