The galaxy presents as a roughly elliptical, concentrated object. It appears to be a relatively smooth galaxy with little evidence of spiral arms or significant dust lanes. The color is predominantly yellow-orange, suggesting a population of older stars. The galaxy is moderately luminous with a redshift indicating that we are seeing it as it was when the universe was much younger. There are no immediately obvious signs of ongoing or recent major merger activity, or major disturbances, but there may be a slight asymmetry that needs further investigation. The central region appears brighter and more concentrated than the outer regions, which gradually fade into the background. Based on its color, morphology and estimated size it is likely a fairly massive system.
