This galaxy appears to be in a late-stage merger. Two distinct nuclei are visible, one slightly brighter and more condensed than the other. A diffuse halo of material surrounds both nuclei, displaying a slight elongation in a roughly east-west direction. The color of the galaxy is primarily yellowish-orange, with a hint of green in the outer regions, possibly indicating some ongoing star formation. There are some disturbances and irregularities in the morphology, suggesting strong gravitational interactions have occurred and continue to occur between the two progenitor galaxies. The tidal tails and bridges of stellar material are not clearly visible in this image, however there seems to be minor disruption in the outer regions of the halo.
