The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy. The light profile suggests a high degree of symmetry. The dominant color is reddish-yellow, indicating an older stellar population with a low rate of ongoing star formation. There is no clear evidence of spiral arms or a distinct disk structure. There may be some faint, diffuse emission surrounding the central region, but it lacks any sharp boundaries or features. There may be a minor gravitational disturbance, possibly from a past minor merger. The object appears relatively round in shape.