The galaxy appears to be undergoing a significant merger event. There are two distinct, luminous cores, suggesting two galaxies in the process of coalescing. These cores exhibit a yellowish-white hue.

The overall shape of the system is highly irregular, with extended, diffuse light surrounding the two cores. This diffuse light suggests tidal tails or disrupted stellar populations resulting from gravitational interactions during the merger. There are no clearly defined spiral arms or a central bulge.

The system's apparent smoothness and lack of sharp features is notable, likely due to the advanced stage of the merger and the distance to the galaxy.

The galaxy system is likely in a relatively quiescent state of star formation.
