The galaxy presents as a somewhat elliptical shape, though it appears closer to a flattened spheroid than a highly elongated ellipse. Its light profile is dominated by a smooth, centrally concentrated bulge that displays a distinct yellow hue.  Fainter and bluer diffuse light extends outward from the bulge, encompassing a larger region, potentially indicative of a disk component. There is no evidence of spiral arms or significant dust lanes.  Overall the galaxy appears as a relatively quiescent object, without major signs of ongoing or recent large-scale merger activity.  There appears to be little active star formation within the galaxy, though the blue light further from the center implies it may be a lenticular galaxy. The luminosity suggests it is a massive galaxy.
