The galaxy presents a disk-like morphology, though it is not perfectly circular. The galaxy appears relatively smooth in overall structure with no apparent spiral arm structure. There is some evidence of minor disturbances. The light profile appears centrally concentrated, suggesting a possible central bulge component. Given the red shift, the object's distance suggests that it is a fairly large galaxy. Overall, the galaxy gives the impression of being a late type spiral or possibly an elliptical galaxy. The color indices may imply that it is a relatively passive system with a low star formation rate.
