The galaxy presents a somewhat disturbed morphology. It appears to be undergoing, or recently underwent, a significant interaction, possibly a merger. The galaxy's core shows a relatively smooth, centrally concentrated structure, possibly an older stellar population. Fainter and bluer regions are observed, suggestive of more recent star formation. A distorted disk-like feature can be inferred, though its structure is severely disrupted. There is no clear spiral arm structure present. Overall, the galaxy displays an irregular and disturbed appearance, indicating a dynamically active history.
