Geometrical and kinematical modeling results as obtained with CANNUBI and ^3DBAROLO. Left panel: Observed CO(4−3) line-velocity integrated map overlaid with the best-fit model. The black and red contours show the [4, 16]σ isophotes of the data and the model, respectively, where σ denotes the noise RMS in the flux map. The dashed gray lines indicate the best-fit location of the major and minor axes of the disk. The white circles show the spacing between the model rings. The ALMA synthesized beam is reported in the bottom right corner. Central and right panels: Position-velocity diagrams along the best-fit major and minor axis of the model. The black and red contours show the [2, 4]σ isophotes of the data and the best-fit rotating thin-disk model, respectively, where σ is the noise RMS per velocity channel.