The galaxy appears as a centrally concentrated object with a smooth morphology. It presents a near-circular shape, showing minimal deviations from roundness. There is no apparent spiral arm structure or significant disk component visible. The overall color suggests a relatively evolved stellar population. No major interactions or signs of ongoing mergers are discernible, although there may be some minor disturbances. The galaxy's apparent size is small, indicating it is a distant object. The concentration of light towards the center indicates it is a relatively massive galaxy. There are no distinct features present, and the galaxy shows no signs of ongoing star formation.
