The galaxy exhibits a complex morphology, appearing to be in a state of interaction or merger. It presents as a diffuse, centrally concentrated object, yet displays significant deviations from a perfectly smooth profile. Two distinct, bright knots are visible within the galaxy's body, potentially indicating the presence of active galactic nuclei or regions of intense star formation within the merging components. 

A faint, irregular halo surrounds the central regions, showing evidence of tidal streams or disrupted stellar material. The overall color of the galaxy suggests a mix of stellar populations, with bluer regions potentially indicating ongoing star formation and redder regions hinting at older, more evolved stars. There is a suggestion of some disk-like structure, but its symmetry is heavily disrupted. It shows considerable irregularities, possibly induced by ongoing gravitational interactions.
