The galaxy appears to be undergoing a significant interaction or merger. Evident are two distinct bright nuclei, potentially indicating the centers of two originally separate galaxies. One nucleus exhibits a yellowish-white color, suggesting an older stellar population or significant dust obscuration. The other nucleus appears more reddish, possibly indicative of active star formation shrouded in dust or a different population of stars.

A faint, diffuse envelope of light surrounds both nuclei, suggesting tidal interactions are disrupting the original structures. The overall morphology is highly irregular and disturbed, with no clear spiral arms or elliptical shape visible. Extended faint features extend outward, further suggesting ongoing gravitational interactions. The system shows evidence of both smooth, blended light and distinct, unresolved sources, possibly star clusters or regions of intense star formation. The overall color is a mix of red and yellowish-white, with a bias towards redder hues.
