Spectral energy distribution comparing the contemporary photometry (blue circles; Table A.1) and the MATISSE spectrum (red; epoch 4) against the analytical (green) and RADMC-3D (black) models with the two disk orientations: ALMA (dashed lines) and MATISSE (solid lines). The bottom two panels are enlargements of the L- and N-band regions. The shaded regions represent the flux uncertainties of the MATISSE spectra, while the 9.4–9.9 µm spectral region is heavily affected by the terrestrial atmosphere.