This galaxy appears to be undergoing a merger, or at least experiencing significant gravitational interaction. One section of the galaxy displays a prominent blue hue, indicative of ongoing star formation. The morphology suggests a disk structure, with an overall irregular form due to possible tidal disturbances. There is a notable concentration of older stars or dust, exhibiting a redder color, possibly representing a more evolved stellar population. The galaxy shows signs of moderate star formation, but not at an extreme rate. The system does not present a particularly smooth or undisturbed appearance, aligning with the merger hypothesis.
