  Super-massive black holes (SMBH) are present at the center of most galaxies,
with the related mass accretion processes giving origin to outflows in Active
Galactic Nuclei (AGN). It has been presumed that only intense winds from
luminous AGN were able to suppress star formation until the discovery of a new
class of galaxies with no recent star formation and with the nucleus in a
quiescent state showing kpc scale outflows. We used SDSS MaNGA and Gemini
Integral Field Spectroscopy of the prototype Red Geyser Akira and found that
the orientation of the outflow changes by about 50$^\circ$ from its nucleus to
kpc scales. A possible interpretation is that the outflow is produced by a
precessing accretion disk due to a misalignment between the orientation of the
disk and the spin of the SMBH. The precession of the central source is also
supported by a similar change in the orientation of the ionization pattern.
Although similar behavior has commonly being reported for collimated
relativistic jets, the precession of an AGN wide wind is reported here for the
first time, implying on a larger work surface of the wind, which in turn
increases the star formation suppression efficiency of the outflow.
