The galaxy appears as a single, concentrated, and relatively smooth object. The light is dominated by a central bulge which exhibits a high degree of symmetry. There is very little evidence of spiral arms, dust lanes, or other distinct morphological features that would indicate ongoing star formation or disk-like structure. The overall color is yellowish-orange, suggesting a population of older stars. The galaxy appears to be somewhat elliptical in shape, although it is close to being circular, with no obvious signs of recent mergers or major disturbances. The light is relatively compact, with no clear extended halo or tidal features.
