The galaxy appears to be undergoing a significant interaction or merger event. There are several distinct components visible, suggesting multiple galactic nuclei or highly disturbed regions. The primary structure is not easily categorized as spiral or elliptical, exhibiting an irregular morphology. A dominant, bright central region displays a greenish hue, possibly indicating intense star formation or an active galactic nucleus. Peripheral to the brighter regions are more diffuse areas with varying colors, suggesting different stellar populations or dust obscuration. Faint extensions or tidal features may be present. The overall shape is complex and asymmetric.
