The galaxy presents a disturbed morphology, likely indicative of an ongoing or recent interaction or merger. It exhibits a complex structure with an apparent tidal tail extending from the main body of the galaxy. The tidal tail appears bluish, possibly suggesting the presence of younger stars formed as a result of the interaction. The main body of the galaxy has a more diffuse, yellowish-red color, potentially indicating an older stellar population. There is a higher concentration of star formation in what appears to be the most disturbed part of the galaxy. Overall, the galaxy does not have a smooth appearance and shows visible signs of an ongoing merger or significant gravitational disturbance.
