The galaxy exhibits a complex morphology, displaying characteristics suggesting an ongoing or recent merger event. There is evidence of significant tidal disruption, with prominent extended features and a disturbed central region. The light distribution appears irregular, lacking a well-defined spiral arm structure or elliptical profile. The color gradients suggest differential stellar populations, with a relatively redder, possibly older population in the central region, and bluer, potentially younger populations distributed in the outer features and tidal tails. There appear to be multiple distinct nuclei or concentrated regions of star formation within the system. The overall impression is that of a dynamic system undergoing significant gravitational interaction, possibly involving multiple galaxies.
