The galaxy presents as a centrally concentrated, relatively smooth object. There is a discernible core region exhibiting higher surface brightness. The overall shape appears largely elliptical, tending toward a spherical morphology rather than a flattened disk. Weak color gradients are observed, with the core slightly yellower than the outer regions. No prominent spiral arm structures or dust lanes are visible. There is no obvious indication of a major ongoing merger event, though subtle disturbances in the outer isophotes cannot be completely ruled out. The galaxy exhibits a moderate degree of blueness, suggesting a non-negligible population of young stars.
