The galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology suggests a lack of significant star formation, corresponding with its low specific star formation rate. It is generally round, without any obvious signs of disturbance or ongoing mergers. The galaxy has a bright core that fades gently towards the edges. Its apparent color is moderately red, suggesting an older stellar population with few young, blue stars. The overall structure suggests a gravitationally relaxed system that has undergone significant evolution.
