The galaxy exhibits characteristics suggestive of a late-stage merger. The morphology is highly disturbed with a distinct lack of a clear, single galactic nucleus. Instead, there are what appear to be two bright knots, potentially representing the cores of the progenitor galaxies, connected by a tidal bridge or stream of diffuse material. These knots display a blueish hue, possibly indicating active star formation within them. Extensive tidal tails and debris surround these main components, indicative of strong gravitational interactions. The spiral arms are not well defined, appearing loose and fragmented, likely disrupted by the ongoing merging process. The overall color gradient suggests a diverse stellar population, with possible regions of enhanced star formation and older, redder populations mixed within the disturbed structure. There's also no clear sign of a prominent bulge.
