The galaxy appears to be in the process of a merger. One component is significantly brighter and more compact than the other. The brighter component displays a somewhat disturbed morphology, possibly exhibiting signs of tidal interactions. It presents a distinct central region with a slightly elongated shape and a predominantly blue/cyan color, suggesting ongoing star formation. 

The second, fainter component is elongated and oriented roughly horizontally relative to the brighter component. Its color is more reddish/yellow, which could be due to older stellar populations and/or dust obscuration. There is a possible tidal tail extending from the edge.
