The galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a concentrated central bulge, with the light intensity decreasing gradually from the center outwards. There is very little evidence of spiral arm structure or dust lanes. The color profile suggests a population of older stars, with a yellowish-red hue dominating the central region and outer regions. There are no indications of strong ongoing star formation. There is also a potential minor disturbance that may or may not indicate an ongoing or recent merger event. 
