The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, bright core, with a gradual decrease in luminosity towards its outer regions. Its overall shape is nearly circular. There is no apparent spiral structure or significant dust lanes visible in this image. The galaxy presents with a slight yellowish hue, suggestive of an older stellar population and minimal ongoing star formation. There is no obvious evidence of any major tidal disturbances or ongoing merger activity. Close inspection reveals no prominent satellite galaxies or other interacting objects nearby.
