This galaxy exhibits a morphology that is suggestive of a late-stage merger event. The main body of the galaxy is elongated and appears diffuse. There are two distinct, brighter knots of light on either side of the central region of the galaxy. These could represent the remnants of the cores of the progenitor galaxies. The overall color of the galaxy is bluish, possibly indicating recent star formation, particularly in the brighter knots. There is some faint tidal debris visible extending from the main body which further supports the ongoing merger scenario. The primary structure appears somewhat disturbed, lacking a clear spiral arm structure.
