  Active galactic nucleus (AGN) outflows including jets and ionized winds have
been key phenomena such as jet collimation and AGN feedback to the host galaxy
in astrophysics. Radio galaxies, a type of AGN with misaligned jets, have
provided valuable insights into the properties and relationships of these
outflows. However, several aspects regarding AGN outflows remain unclarified,
such as the relationship between jets and ultrafast outflows (UFOs) and the
differences between the properties of radio-loud AGN disk winds and radio-quiet
AGN ionized winds. To clarify these aspects, radio galaxies containing UFOs and
warm absorbers (WAs) must be studied. Currently, both UFOs and WAs have been
reported in only two radio galaxies, 3C 390.3 and 4C $+$74.26. To enhance our
understanding of the connection between the jets and ionized winds, we
conducted a study on Mrk 6, a potential candidate for the third case of a radio
galaxy displaying these characteristics. Using X-ray spectra obtained from {\it
XMM-Newton}, we performed photoionization modeling using the SPEX code. The
best-fit model analysis results revealed the presence of a UFO component with a
relatively low ionization parameter (Fe {\sc xix}/{\sc xviii} lines blueshifted
by $-34700^{+400}_{-200}~{\rm km~s^{-1}}$) and a WA component with an outflow
velocity of $-7600 \pm 200~{\rm km~s }^{-1}$. To further confirm the nature of
the UFO and WA in Mrk 6, we simulated the X-ray imagining and spectroscopy
mission spectra.
