The galaxy exhibits a complex morphology, appearing to be in a state of interaction or merging. One dominant, relatively smooth component shows a somewhat amorphous, diffuse structure with a bluish hue, possibly indicating regions of recent star formation. There appear to be multiple nuclei present, or perhaps highly luminous star clusters within the larger system. There is evidence of tidal features or distortions, possibly indicative of gravitational interactions. The redder light emanating from the core region is concentrated and tightly packed. There appears to be a dust lane that obscures some of the structure of the galaxy, and is highly luminous in orange and red light.
