Continuum emission from the R100 JWST/NIRSpec datacube. From left to right the average continuum emission between 1–2 μm (1530–3058 Å rest-frame), 3.3–4.2 μm (5045–6422 Å rest-frame), 4.4–5.2 μm (6730–7950 Å rest-frame), respectively. The magenta circles represent the apertures from which we extract the spectrum for the north, central, and southern components for the analysis. The black contours represent the [O III] emission at 5, 25, and 75σ (see Fig. 1). The black cross shows the location of the [C II] emission peak (see Fig. 1). The x and y axes represent the displacement in arcsec with respect to the galaxy center (RA = 09h58m28.5s, Dec = +02d03m06.7s, see Sect. 1).