  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 to 600-700 km/s,
respectively, on the radial distances of ~2.5 and ~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.
