The galaxy appears to be an irregular type, exhibiting a disturbed morphology. There are features suggesting an ongoing or recent interaction or merger. Evident are tidal tails or extended structures of diffuse material extending outwards from the main galactic body. These appear bluish, indicative of recent star formation.

The main body of the galaxy shows a somewhat clumpy structure, with an apparent central concentration that appears more yellow/orange in color, possibly indicating an older stellar population or significant dust obscuration. The overall light distribution across the galaxy is uneven, lacking a clear spiral arm structure or elliptical shape. 

There is an indication of active star formation within localized regions across the disk. The morphology is complex, with no clear single classification being immediately apparent; it could be a late-stage merger remnant, a strongly interacting galaxy system, or an intrinsically irregular galaxy undergoing significant internal processes.
