The object is a galaxy exhibiting characteristics of a late-stage merger. The overall morphology is highly disturbed, showing irregular features and a lack of a defined shape. There are multiple bright clumps of light within the galaxy, indicating possible concentrations of stars or active galactic nuclei. The galaxy displays a range of colors, with some regions appearing bluer, possibly indicating recent star formation, while others are redder, potentially representing older stellar populations. There is no clear indication of a disk structure. Tidal tails or bridges appear to be present. The galaxy has a prominent central bulge, but it is hard to discern if it has any spiral arm structure. The outer regions of the galaxy fade into the background, suggesting a lower density of stars in the halo.
