The galaxy presents as a system undergoing a significant merger. Several distinct luminous clumps are visible, indicating either multiple galactic nuclei or regions of intense star formation triggered by the interaction. The overall shape is highly disturbed, with little to no discernible spiral structure or elliptical symmetry. The primary color appears to be a yellow-red hue, potentially indicating an older stellar population and/or significant dust obscuration. There are some hints of blue on the outer edges of the galaxy, suggesting some regions of newly formed stars. The galaxy is relatively compact.
