The galaxy presents an asymmetrical morphology, suggestive of either a recent or ongoing interaction or merger. Two primary components are discernible. One component exhibits a smoother, more diffuse appearance with a yellowish hue. The other component is more compact and appears distinctly redder and brighter. Faint extensions emanate from the diffuse yellowish component. The overall structure suggests some level of disturbance with light emissions. No distinct spiral arms are visible.
