The galaxy appears to be a relatively small, elliptical galaxy, potentially at a significant distance. Its color is predominantly red, suggesting an older stellar population with a low rate of recent star formation. The overall structure is smooth and lacks any obvious spiral arms or a distinct central bulge. The galaxy is generally round in shape, with only a slight deviation from perfect circularity. There are no immediately apparent signs of a major ongoing merger, but a minor disturbance cannot be ruled out.
