This galaxy presents as a merging system, exhibiting two distinct nuclei separated by a relatively short distance. Each nucleus shows a concentrated central bulge, with surrounding diffuse light indicative of a stellar halo. There is evidence of tidal distortion of the surrounding halo, potentially suggesting an ongoing interaction between the two galaxies. Overall, the system's morphology indicates a late-stage merger event, where the individual galactic structures are still distinguishable, but gravitational interactions are actively reshaping their forms. The color is generally yellow.
