The galaxy appears to be an irregular morphology, with a clumpy and disturbed structure. There is no apparent nucleus, and it does not have the distinct spiral arms of a spiral galaxy, nor the smooth elliptical shape of an elliptical galaxy. It seems likely that the galaxy is currently undergoing or has recently undergone some type of interaction. There is significant patchiness throughout. Some of this is due to star forming regions. Blue hues are prominent within the main body, indicative of relatively young stellar populations. Overall, the galaxy is relatively small.
