This galaxy appears to be part of a merging system, potentially undergoing a significant interaction with a companion. One primary component exhibits a smoother, more diffuse morphology, with a somewhat rounded shape. This component displays a bluish hue, suggestive of a population of younger, hotter stars.

The second component is more compact and shows a distinctly yellow to reddish coloration. The presence of this redder color hints at an older stellar population or significant dust obscuration. The interaction between the two galaxies seems to be causing some degree of tidal disturbance. It also seems that the system is either the result of a merger or the early stage of one.

