The galaxy presents as a system undergoing a significant merger event, likely in its late stages. The core of the galaxy shows a prominent dual nuclei structure. There appears to be a primary, more dominant nucleus and a secondary nucleus close in proximity. 

The overall shape is disturbed and irregular, lacking defined spiral arms or a clear elliptical structure. There is a broad, diffuse halo surrounding the central region. Patches of blue suggest the presence of some star formation. There are some dust lanes and tidal tails. The galaxy appears to be about 8.6 kiloparsecs across.
