The galaxy presents as an interacting system. One component exhibits a smoother, more concentrated morphology with a greenish hue, suggesting active star formation or an active galactic nucleus. The other component is less defined, appearing as a fainter, elongated structure with a bluer color, possibly indicative of a disk or tidal tail. The overall structure of the system shows signs of gravitational disturbance, with potential tidal features extending away from the main bodies. The system appears to be in the process of merging, with significant morphological disruption. There's an indication of dust lanes or obscuration within the fainter component.
