The galaxy presents a complex morphological structure, appearing to be in a late-stage merger. The central region exhibits high luminosity, possibly indicative of active galactic nuclei or intense star formation. Evident tidal tails extend outwards, curving away from the main body. The structure of the galaxy is significantly disturbed, with no clear spiral arm structure, but the shape suggests a disk morphology before the merger event. There are some regions that are distinct in color and shape in the galaxy. The galaxy has an estimated size of around 7.5 kiloparsecs.