The galaxy presents a morphology that is most likely the result of an ongoing or recent merger event. Two primary, relatively bright, yellow-orange galactic nuclei are visible, suggesting that these were the cores of the progenitor galaxies. The overall shape of the system is irregular, with a lack of defined spiral arms or a smooth elliptical profile. There appears to be a diffuse halo surrounding the main body of the galaxy, which is likely composed of tidal debris resulting from the gravitational interactions. The color indices suggest a galaxy composed of older stellar populations.
