This galaxy presents a complex morphology indicative of significant gravitational interaction. The structure appears as a distorted disk, potentially a spiral galaxy, but with disrupted arms. There is an asymmetrical distribution of luminous matter. The primary body of the galaxy does not exhibit a clearly defined nucleus, implying a relatively small or non-existent bulge component. One portion of the main body appears thicker and more diffuse, indicating a possible ongoing merger. There is little evidence of a bar structure, and a complex morphology, but it also appears to have noticeable spiral arms.
