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Fig. 1.

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Left: Composite image showing F200W (blue; stellar continuum), continuum-subtracted H2 1– S(1) from F212N (green), and F770W (red; tracing PAH 7.7 μm emission). The LOFAR 144 MHz radio contours are overlaid. The NIRSpec and MIRI Channel 4 fields of view are shown with cyan and yellow dashed lines, respectively. Right: Zoom-in highlighting warm molecular gas traced by H2 S(9) (green), S(1) (red), and CO 2-1 (blue). Overlaid contours are C band from VLA (white) and MERLIN (black). Key regions are labeled, including the northern and southern dust lanes as well as shocked regions to the northeast and southwest. Physical scale bars are shown in both panels.

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