Model spectrum (black line, generated in a varying resolution across the wavelength range) is overplotted with the observed MIR JWST spectrum (orange line), optical photometric fluxes (blue vertical lines), and millimetre band fluxes (red circles). The MIR Spitzer spectrum (grey line) is shown as well for comparison. Inset plot: Fitting of the MIR continuum, along with the observed AIBs at 6.2, 8.1, and 11.3 μm, and the model generated continuum with the respective PAH bands, is shown in more detail.