The galaxy exhibits a morphology indicative of a disturbed system. The primary body appears somewhat amorphous, lacking a clearly defined spiral or elliptical structure. There is evidence of tidal features or debris extending from the main galactic body. One or more of these features appear to be streams of material pulled away from the galaxy. The color distribution suggests varying stellar populations or dust content within the galaxy. The image suggests that it may be undergoing or have recently experienced a merger event or close interaction with another galaxy.
