The galaxy presents as a merging system, exhibiting significant morphological disturbance. There are two primary concentrations of light, the larger of which exhibits a yellow hue, suggesting an older stellar population. The smaller concentration is whiter in color, which is possibly indicative of ongoing or recent star formation. There are tidal tails present around the main body of the galaxy. The shape of the galaxy is highly irregular, with no defined spiral or elliptical structure visible, indicating a dynamically active system with likely recent or ongoing gravitational interactions. Given the overall disturbed morphology, the system is most likely in the late stages of a major merger. Star formation is suppressed, with few blue stars visible.
