The galaxy presents as a centrally concentrated, elongated structure. There's a high degree of central brightness, suggesting a significant concentration of older stars in the bulge. The galaxy appears relatively smooth with a slight asymmetry. The overall color suggests a mix of stellar populations with a tendency toward redder hues. No spiral arm structures or prominent dust lanes are clearly visible. There may be some evidence of tidal disturbances, but the galaxy appears to be mostly isolated and well-formed. Overall, this galaxy appears as a medium-sized elliptical galaxy that may be undergoing some minor mergers or tidal disruptions.
