The galaxy exhibits a spiral morphology, presenting with loosely wound spiral arms. Two prominent and active galactic nuclei are visually apparent, suggesting this object is likely the result of a recent or ongoing galactic merger. A substantial degree of tidal disruption is observed; this evidence leads to classifying it as a major merger. The galaxy displays a somewhat disordered structure, indicative of strong gravitational interactions. The color gradients suggest variations in stellar populations across the galactic structure, with bluer regions potentially correlating to areas of more recent star formation activity within the spiral arms. A less prominent bulge size is also seen. The spiral arms appear asymmetrical.