This galaxy exhibits a morphology that suggests it is undergoing a merger or tidal interaction. The primary body of the galaxy appears somewhat diffuse, lacking a sharply defined core or spiral arm structure. There is a distinct, elongated shape with a brighter, concentrated region that may represent the remnant nucleus of one of the merging galaxies.

Evidence of disturbed morphology is present in the form of faint, extended tidal features or irregular structures extending outwards from the main body. These features have a bluer color, indicating the presence of younger stars. The overall color gradient suggests active star formation in some regions, potentially triggered by the gravitational interactions.
