The galaxy presents as a complex system, likely undergoing a significant interaction or merger event. There appear to be multiple components, possibly two or three distinct galactic nuclei or dense star clusters. One component exhibits a smoother, more diffuse light profile, suggestive of an elliptical or spheroidal morphology. Another appears more compact and possibly disk-like, though heavily disrupted, displaying a bluer color indicative of younger stellar populations. There's evidence of tidal features, such as faint streams or distortions, implying gravitational interaction between the galaxy components. The overall color is relatively blue, hinting at ongoing star formation activity, although the presence of a redder, potentially older stellar population is also suggested in some regions. There is a clear disturbance to the disk, if there is one, with no clear spiral arms. Overall the galaxy seems to be in a state of flux. 
