The galaxy presents as a luminous, centrally condensed object. Its morphology is predominantly smooth, with a slight elongation suggesting it is not perfectly spherical. The galaxy exhibits a light blue hue in the central region, which could indicate recent or ongoing star formation. A minor reddish area is observed on one side, potentially indicative of a region of older stellar populations or dust obscuration. There are no obvious signs of strong tidal features or distortions that would immediately suggest a major ongoing merger, although minor disturbances cannot be ruled out.
