The galaxy presents as a roughly elliptical morphology, appearing mostly smooth with a bright central bulge. Its color suggests a population of older stars, though there are hints of bluer regions, suggesting the presence of some younger stellar populations or star formation activity. The galaxy appears to be relatively isolated with no obvious signs of interaction or tidal disturbances in this image. The galaxy's overall structure indicates a relaxed system, with no strong evidence of recent mergers or significant ongoing star formation. The light distribution is centrally concentrated, fading gradually toward the outer regions.
