The galaxy exhibits a morphology that appears largely smooth and elliptical. Its overall shape can be described as somewhere between round and oblong. There are possible signs of a faint disk. Light emitted across the optical spectrum is dominated by redder wavelengths, indicating an older stellar population. There may be a low level of ongoing star formation, but it is relatively quiescent overall. There is visible disturbance in the structure of the object and it is possibly merging. The galaxy is a high mass galaxy.
