The galaxy presents as a complex, multi-component system, possibly undergoing a merger or strong interaction. There appear to be at least four distinct luminous cores arranged in a roughly vertical configuration. The brightest of these cores exhibit a yellowish-orange hue, suggestive of an older stellar population. 

Extending outwards from these cores is a faint, diffuse halo of light. A subtle gradient in color is observed within this halo. The lower portion shows hints of bluer emission, possibly indicative of regions of more recent star formation. The general morphology leans towards a more spheroidal or elliptical shape, although the ongoing interaction likely distorts any pre-existing structure. There may be tidal tails present.
