This galaxy appears to be undergoing a significant merger event. Two distinct galactic nuclei are visible. The northern nucleus presents a more diffuse, yellowish-orange color. The southern nucleus is brighter and exhibits a bluish-white hue, possibly indicating a region of active star formation. There is a slight green tint near this nucleus as well. Overall, the morphology suggests that the galaxy is disturbed. The shape appears neither perfectly elliptical nor spiral, displaying a more irregular form indicative of gravitational interactions. There is evidence of tidal forces acting on the galaxy, potentially resulting in streams or plumes of stellar material, although such features are subtle in this image. Further spectroscopic analysis is needed to confirm the nature of the nuclei and the dynamics of the merger.
