The galaxy appears to be largely smooth and elliptical in shape, lacking any prominent spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, showing a gradual decrease in intensity outwards from the core. The galaxy exhibits a generally round morphology, with minimal elongation or asymmetry. There are no obvious signs of major mergers or significant tidal disturbances. The overall color suggests a population of older stars with some younger bluer populations mixed in.
