This galaxy appears to be undergoing a major merger. There are two distinct, luminous clumps that are approximately the same size, the lower clump is noticeably larger. These clumps likely represent the original galactic nuclei of the merging galaxies. A faint tidal tail extends outward from one of the clumps, suggesting a strong gravitational interaction and distortion of the original galactic structures. The overall morphology is heavily disturbed and lacks a clear disk structure. The color of the galaxy is generally yellow, implying an older stellar population.
