  NGC 1068 is a nearby Active Galactic Nucleus (AGN) of type 2, meaning that
its accretion disk is hidden behind a large amount of foreground extinction.
Observations at several wavelengths have revealed various disk-like structures
around the nucleus, all possibly part of the putative torus responsible for the
obscuration of the AGN. The paper presents results based on GRAVITY/VLTI
interferometric observations in the near-infrared, which provide very high
angular resolution, and gives insights into the geometry of the innermost
region of the torus. The 3D orientation of the structure is surprising in
several aspects, as it is misaligned with other disks present around the
nucleus, and leaves a clear line of sight toward the central source.
