The galaxy appears to be in a state of interaction or recent merger. There are two distinct bright nuclei, indicating either two distinct galaxies or a single galaxy with a double nucleus due to an ongoing merger event. 

The overall morphology is disturbed, lacking a clear spiral or elliptical structure. There is a diffuse, extended halo surrounding the main body of the galaxy.

Based on the bluer color, at least one of the nuclei shows evidence of ongoing star formation. A redder component is present, possibly indicating an older stellar population. 
