The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated luminosity profile. The core is bright and yellowish-white, indicating a significant population of older stars. There is a gradual decline in luminosity moving outward from the core, forming a diffuse halo. A subtle bluish tint surrounds the central region, suggesting the possibility of some younger, star-forming regions, although the overall color indicates that the star formation rate is likely low. The shape is approximately round, with no obvious disk or spiral arm structures. There is no immediately apparent evidence of tidal tails, mergers, or other significant disturbances. The galaxy exhibits a smooth overall appearance, with no pronounced features, indicating it is likely an evolved system.
