Spectra extracted from the kiloparsec-scale disk. Line profiles of H₂ (top) and Paα (bottom) at the position of the three spaxels labeled in Fig. 12. The black dashed curves represent the spectra from the original cube, highlighting the contribution attributed to the HGO and SEO (red-shaded area) that we have already isolated and subtracted; the black solid lines represent the spectra fitted to identify the large-scale disk. The red dashed curves show the components associated with the disk model. The total disk model is shown with a solid red curve. Velocities are computed with respect to z_m.