The galaxy presents a relatively smooth and concentrated light profile. It appears to be elliptical in shape, displaying a largely spheroidal structure with high degree of central concentration. There is minimal evidence of spiral arm structure or significant dust lanes; any features beyond a smooth central structure are subtle. Color analysis suggests a somewhat redder stellar population throughout the galaxy. There is no dominant central bulge; it has a mostly uniform color and luminosity. The galaxy appears to be isolated; with no bright companion galaxies or significant tidal disturbances readily apparent in this image.
