The galaxy appears as an elliptical-shaped object with a smooth, diffuse light distribution. The central region is bright and concentrated, exhibiting a yellowish hue. The galaxy's light gradually fades towards its outer edges, which blend smoothly into the background sky. There is little evidence of distinct spiral arms or prominent features. The overall color suggests an older stellar population, though some bluer regions indicate possible ongoing star formation. The symmetry and lack of significant tidal features suggest it is not currently undergoing a major merger. There are some minor disturbances potentially present, although these could also be due to image limitations. The galaxy's shape is somewhere in between round and cigar shaped.
