The galaxy appears to be a relatively smooth, elliptical system with a dominant, bright central bulge. The overall color is yellowish, suggesting a population of older stars. There is no clear evidence of spiral arms or a prominent disk structure. The outer regions of the galaxy fade gradually, indicating a diffuse halo. The apparent lack of dust lanes or prominent star-forming regions suggests a low star formation rate. The galaxy exhibits a generally relaxed morphology, without obvious signs of recent mergers or tidal disturbances. It presents as a single, mostly homogenous light source.
