The galaxy appears to be undergoing a merger. There are two distinct, bright nuclei visible, indicating the presence of two separate galaxies in close proximity and gravitational interaction. The overall morphology is disturbed and irregular, lacking a clear spiral or elliptical structure. There is an observed smoothness to a significant portion of the galaxy, particularly in the areas surrounding the nuclei, but there are also hints of tidal features. The galaxy exhibits a redder color, possibly indicating an older stellar population or significant dust obscuration. Some blue regions exist as well. There is evidence of star formation within the merging system, particularly in the bluer parts of the structure.
