The galaxy presents a somewhat disrupted morphology. The central region exhibits a bright, slightly elongated concentration of light, possibly indicating a bulge component. From this central region, faint spiral arms appear to extend. A significant portion of the galaxy's light seems concentrated in these arm structures. There appear to be several regions of active star formation within the arms, visible as knotty regions of bluer light. Overall, the galaxy does not show a well-defined, symmetrical structure, suggesting a potential gravitational interaction or recent merger event, as the morphology appears disturbed.
