NGC 424 rotation curve inferred with MOKA^3D using the H₂S(1) (orange) and CO (2-1) (green) emission, and the narrow component of the [O III] (blue) emission line, from MIRI/MRS, ALMA, and MUSE, respectively. The rotation curve obtained fitting the narrow component of the [Ne III] shown in Fig. 4 is not reported, as the trend is similar to the H₂S(1). The dotted black and grey curves represent the best-fit velocity profile of the DM (Eq. (3)) and baryonic matter (Eq. (2)), respectively. The total best-fit profile is shown as a solid red curve. The averaged rotating velocity and inclination values are listed in Table 2. Details on the MOKA^3D disc model are discussed in Sect. 4.1.