The galaxy appears to be a relatively luminous elliptical galaxy. Its morphology is predominantly smooth and spheroidal, with a concentrated, bright central bulge that diffuses outwards, and a less structured halo. The color gradient shifts from a yellow-orange core region to a blue-green outer region. There is very little evidence of prominent spiral arms or dust lanes. The overall structure suggests a system that has undergone significant dynamical relaxation. There are some possible faint disturbances in the halo that could be evidence of minor interactions. The galaxy seems to be isolated and not currently undergoing a major merger event.
