The galaxy appears as a centrally concentrated, relatively smooth object with a faint, diffuse halo. The light is generally uniform, indicating it is likely an elliptical or lenticular type galaxy. There is a slight elongation, suggesting a possible cigar shape. There are no obvious spiral arm structures or significant dust lanes visible in the image. There is no evidence of a major ongoing merger, though a minor disturbance is not ruled out. The overall color is yellowish, which may indicate an older stellar population.
