The galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent interaction. There is a central, somewhat amorphous structure from which faint, diffuse tidal features appear to emanate, suggesting gravitational interaction. These features extend outwards. The overall color of the galaxy is relatively uniform, with subtle variations in intensity that could suggest differing stellar populations within the system. Given the disturbed morphology, a minor or major merger classification seems plausible, based on the faint and diffuse, wispy morphology, and lack of a central, clear spherical shape.
