The galaxy presents as a complex system, possibly undergoing a merger or exhibiting strong tidal interactions. The primary body of the galaxy appears diffuse, lacking a well-defined spiral structure or elliptical shape. There is a dominant, reddish-orange core suggestive of an older stellar population. Emanating from this core are fainter, irregular extensions of bluer material, indicating regions of active star formation. These extensions might be indicative of tidal tails or disrupted galactic arms. The overall morphology is disturbed, with indications of multiple components merging together. There is a notable, bright blue region, that could be a star forming region, or perhaps a more compact object within the galaxy. The light from the galaxy appears moderately redshifted, indicating a substantial distance. Given the disturbed morphology and presence of star formation, the system likely experiences ongoing dynamical processes.
