The galaxy presents a concentrated, predominantly smooth morphology, with a centrally dominant bulge-like structure. The color gradient suggests a stellar population that is comparatively older and redder in the central regions, with younger, bluer stellar populations possibly present in a more localized area, potentially indicative of ongoing star formation, or perhaps tidal features. There's a clear asymmetry with a defined extension, suggesting the potential for a recent interaction. The overall shape is generally round, though with some irregularities that may imply tidal interactions or an unsettled state. The high concentration of light in the core suggests it's a massive galaxy.
