This galaxy exhibits a morphology suggestive of an ongoing or recent merger event. Evident are significant tidal distortions and disruptions to the expected galactic structure. A substantial portion of the light is concentrated within two relatively bright, somewhat ill-defined cores, potentially representing the nuclei of the merging galaxies. These cores appear embedded within a larger, diffuse halo of light, indicative of the combined stellar populations and gas expelled during the interaction. While the system displays some hints of spiral structure, the overall form is highly irregular, obscuring any clear classification. The colours appear to be primarily composed of older stellar populations.
