We present an analysis of 3D spectra of Mrk 533 , observed with the integral-field spectrograph MPFS and using the Fabry Perot Interferometer ( FPI ) of the SAO RAS 6-m telescope .
We found emissions of gas from the active Sy 2 nucleus in the centre and also from the HII regions in a spiral structure and a circumnuclear region .
The gas kinematics shows regular non-circular motions in the wide range of galactocentric distances from 500 pc up to 15 kpc .
The maps of inward and outward radial motions of the ionized gas was constructed .
We found that the narrow line region ( NLR ) is composed of at least two ( probably three ) kinematically separated regions .
We detect a stratification in the NLR of Mrk 533 with the outflow velocity ranging from 20-50 km s ^ { -1 } to 600-700 km s ^ { -1 } , respectively , on the radial distances of \sim 2.5 and \sim 1.5 kpc .
The maximal outflow velocity comes from the nucleus and corresponds to the position of the observed radio structure , which is assumed to be created in an approaching jet .
We suggest that these ionized gas outflows are triggered by the radio jet intrusion in an ambient medium .