The galaxy appears as a somewhat centralized object with a moderate level of overall structure. It exhibits a morphology that leans towards smooth, but contains some more complex characteristics.

The general form of the galaxy is somewhat elliptical. It has no obvious spiral arm structure, but shows some irregularity in its overall light distribution, suggesting it is not a simple elliptical galaxy. A fraction of the light is slightly bluer, suggesting some level of on-going star formation. The galaxy is neither a pure elliptical nor a late-type spiral but is more likely to be an intermediate type galaxy. There is no apparent major merging or strong tidal distortion; however, a minor disturbance cannot be ruled out. 
