The galaxy appears to be an elliptical morphology, although there are certain indications that it is an interacting system. The central bulge region exhibits a diffuse, smooth light distribution indicative of an older stellar population. There appears to be tidal tails present, as well as some irregular features.

Given its redshift, this is a considerably large and massive galaxy. The colour distribution is relatively uniform and is more red, which may suggest a more evolved system with reduced star formation. The presence of the tails is highly indicative of some kind of merging history. 
