Possible geometries for the CND in MCG -01-24-012. The legend from Fig. 8 also applies here. The left and right columns show the observation and lateral views, respectively. On the right, we added arrows to represent the velocity vectors of the components c1 (blue) and c2 (orange), decomposed in the rotating (bluish-green) and outflowing (black) parts, with diagrams. As in Fig. 8, the orientations of the ionized cones were chosen to try to reproduce the [O III] emission (reddish-purple contours). In the first row, the face-on CND is the result of fitting a rotating disk model with free PA. In this scenario, the CO double peaks would result from expanding clouds perpendicular to the disk. In the last row, we show another way of reproducing the double peaks by assuming an edge-on disk geometry, with the outflow occurring radially along the disk. Our preferred scenario lies between these two geometries, as shown in the middle row. This model is the result of fixing PA at 0° to reproduce the CO flux distribution, which yields an inclination of 74°.