A revised version of the kinematic model of the NLR, first proposed by Tecza et al. (2001) and Cecil et al. (2002), which now accounts for the molecular outflow (denoted in figure as CO outflow) detected by ALMA in the CND (seen in projection in N and S, for northern and southern knots) and farther north in the molecular disk. The figure shows a crosscut of the NLR as viewed from inside the galaxy disk along the projected direction of the radio jet (PA ~ 30°; shown by the green line). We highlight the extent of the ionized gas outflow (light purple shade) and the assumed geometry defined by angles α and i.