The galaxy exhibits a disturbed morphology suggestive of a possible interaction or merger event. Two distinct luminous regions are apparent. The top region has a smoother appearance with a more yellow tint, suggesting an older stellar population. The bottom region appears bluer and more diffuse. There is a general roundness to each region, with a slight elongation. Overall, the galaxy appears to be intermediate in color. Some asymmetry can be noted in both regions. A tail or bridge cannot be seen between the regions.
