The observed galaxy presents as a relatively smooth, elliptical morphology with a notable red color index. The object appears quite round. There may be a very minor disturbance in the morphology. A second object is also within close proximity and may be actively merging. The galaxy's redshift suggests it is a considerable distance away. Given its apparent magnitude and estimated distance, this galaxy is intrinsically luminous. Overall, this object appears to be a massive, relatively quiescent galaxy potentially undergoing a merger.
