The galaxy presents a relatively smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual decrease in intensity towards the outer regions. The galaxy appears quite round. There is little evidence of spiral arm structure or significant dust lanes. Based on its color, the galaxy likely contains an older stellar population. There might be a small amount of minor gravitational disturbance, but overall the system does not show signs of a major ongoing merger event. Given its size, the galaxy is likely quite massive, and is experiencing a low amount of star formation.
