The galaxy appears as a singular object that is smooth in appearance with some possible features present. The light is more centrally concentrated than spread across an obvious disk. There is a slight color gradient from a yellower center to bluer edges. The galaxy is neither perfectly circular nor highly elongated. It seems to be of considerable mass, exhibiting low levels of star formation. There are some visible signs of minor disturbances within the galaxy. There is some evidence suggesting ongoing or past merger events.
