The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. Its shape is moderately elongated, appearing as a flattened spheroid. There are no clearly defined spiral arms or dust lanes visible. The galaxy's color appears to be a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars and a relatively low rate of ongoing star formation. The galaxy's integrated light suggests it is a massive galaxy. There is some evidence of minor gravitational disturbance of the galaxy. There does not appear to be any major mergers or any artifacts. 
