The galaxy appears to be undergoing a significant merger event. There are two primary bright cores visible, suggesting either two distinct galaxies in the process of colliding and merging, or a single galaxy with a highly disturbed morphology due to a recent interaction. The morphology is irregular and shows signs of tidal disruption. A faint, elongated tail-like structure extends from the main body of the galaxy, possibly composed of stars and gas ejected during the merger. The overall color of the galaxy is relatively blue, indicating the presence of ongoing or recent star formation. The distribution of light is uneven, with clumps and knots visible across the galaxy, suggestive of intense star-forming regions triggered by the gravitational interaction.
