This galaxy appears to be a complex system, possibly undergoing a merging event or exhibiting signs of past interactions. The overall morphology is irregular and disturbed, with a notable absence of a well-defined spiral structure or elliptical shape.

There are several distinct, bright clumps of emission visible across the galaxy's extent. These clumps exhibit a range of colors, with some appearing more yellow-white, suggesting older stellar populations, and others showing reddish hues, potentially indicating regions of active star formation obscured by dust. 

The galaxy's light is not uniformly distributed. The core region seems to be brighter and more compact with a bright center, indicating higher stellar density or an active galactic nucleus. Emanating from this central region, less dense filaments of light extend outwards. A slight tidal tail feature could be present, suggesting gravitational interactions or a recent merger.
