The galaxy presents a morphology that suggests it is in a state of interaction or disturbance. It exhibits a central bright region which then fades into a diffuse halo. The light is bluer in color, indicative of ongoing or recent star formation. This galaxy shows hints of tidal tails or disrupted structures, evidenced by the irregular shape and extensions of light emanating from the central region. This galaxy is not particularly well-defined, which indicates a possibility that it's undergoing significant gravitational interactions with another galaxy, even if a merger is not fully underway. This system may be undergoing a merger, where one of the galaxies in the merger is much smaller than the primary galaxy.
