The galaxy appears as a centrally concentrated, generally smooth, elliptical morphology. The light profile suggests a relatively old stellar population, emitting primarily in the redder wavelengths. There is a slight elongation in the shape, but it is mostly round. No obvious tidal features or signs of major mergers are apparent within the limitations of the image resolution. There are no clear spiral arms, dust lanes, or prominent star-forming regions discernible. The overall appearance indicates a galaxy that is not actively undergoing significant star formation, and is likely to be a massive galaxy. 
