The galaxy exhibits a somewhat amorphous structure with a moderate degree of central concentration. The overall light distribution appears relatively smooth, however, there are several areas of enhanced luminosity. It is difficult to resolve any distinct spiral arms or a clear disk structure. There is a suggestion of a diffuse envelope surrounding the main body of the galaxy. There appears to be significant disturbance in the morphology of the galaxy. The object seems likely to be either undergoing a merger or is an artifact. 
