The galaxy presents as a yellowish-orange, elliptical-like structure. It exhibits a smooth, centrally concentrated morphology with a relatively high degree of roundness. There is no discernible disk or spiral arm structure. The galaxy appears largely undisturbed, showing no strong evidence of ongoing or recent major merger activity, although there may be some minor asymmetry. It's color indicates an older stellar population, with relatively little ongoing star formation. The red shift indicates the galaxy is at significant cosmological distance.