  We use a 3D photoionization modeling tool to study the morpho-kinematic
properties of the Planetary Nebula (PN) NGC 3132. We show that it is possible
to reproduce the low resolution observations (spectra and images) with an
ellipsoidal shell. However, high resolution observations, as those showing a
density variation along the nebula and the [O III]5007 velocity profiles,
definitively rule out this description. We show that a bipolar Diabolo shape
with a 40 degres rotation of the symmetry axis relative to the line of sight
successfully reproduces the observed images, as well as the high resolution
observations.
