The galaxy appears as a relatively smooth, elliptical object. Its color suggests an older stellar population with minimal ongoing star formation. The galaxy's shape is largely featureless, exhibiting a gradual radial decrease in luminosity. There is little evidence of spiral arms or prominent dust lanes. The observed light is likely dominated by evolved stars, and there are no visually discernible signs of recent or intense merger activity. A slight asymmetry may indicate past interaction or a minor disturbance, but the overall structure suggests a relaxed system.
