The galaxy exhibits a complex morphology, appearing to be in a late-stage merger. Two distinct luminous cores are visible, indicative of the nuclei of the merging galaxies. The upper core appears more compact and spheroidal, exhibiting a yellow-white hue suggesting an older stellar population. The lower core appears more diffuse with a similar yellow-white hue. A tidal bridge or shell-like structure with a bluish tint connects and surrounds the two cores, suggestive of ongoing tidal interactions and potential star formation. The overall shape is irregular, lacking any defined spiral arms or a smooth elliptical profile. Minor disturbances are present, likely remnants of the merger process. The luminosity suggests a galaxy of significant mass.
