The galaxy presents as a centrally concentrated, smooth object, generally elliptical in shape, with a slight elongation. The color profile is dominated by yellow-red hues, suggesting an older stellar population and/or significant dust content. There is no obvious spiral structure, and the morphology appears relatively undisturbed, with a distinct lack of tidal tails or other indications of recent major merger activity, but some minor disturbances are apparent. The galaxy appears relatively compact. The overall impression is that of a mature, relatively massive system with ongoing, but limited, star formation.
