The galaxy exhibits a disturbed morphology, suggesting an ongoing or recent interaction. The primary body of the galaxy presents a somewhat irregular shape, lacking a clear spiral arm structure. It appears to be undergoing a major merging event and presents significant disturbances to the disk. There is evidence of tidal features or plumes extending away from the main body, which could indicate gravitational disruption. The color distribution within the galaxy is not uniform; there are bluer regions, potentially indicating areas of active star formation, as well as redder regions, possibly older stellar populations. Overall, the galaxy appears to be in a dynamic state, and further spectroscopic analysis would be beneficial to fully characterize its properties.
