The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a high degree of central concentration with a bright core. There is a gradual decrease in luminosity from the center outwards, with no apparent spiral arm structure or distinct features. The galaxy's shape is mostly round with a slight hint of elongation. There is no noticeable dust lane or significant tidal disturbance indicating recent major merger activity. The galaxy's overall color appears somewhat redder, potentially indicating an older stellar population and a lower rate of ongoing star formation. The galaxy presents as a single, unified structure with no signs of a current or recent merger in progress.
