The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is elliptical, exhibiting a high degree of roundness with minimal elongation. There is a subtle color gradient, transitioning from a slightly bluer core to redder outer regions. This may suggest a population of younger, hotter stars in the core with older stars in the outer areas. The smoothness indicates a lack of significant spiral arm structure or large-scale irregular features. The lack of obvious tidal tails or other distortions suggests that this galaxy has not undergone a major merger recently, although there may be minor disturbances or interactions causing the slight asymmetry. The light distribution gradually decreases from the center outwards, implying a lack of prominent star-forming regions outside of the central area.
