The galaxy presents as a generally smooth, elliptical structure. A central bulge, exhibiting a yellowish-orange hue, dominates the core region, suggesting a population of older stars. The galaxy lacks any discernible spiral arm structure. The outer regions of the galaxy fade into a less distinct halo, with a slight bluish tint, suggesting some presence of younger stars. There are no significant signs of any major mergers or tidal disturbances.
