  Active galactic nucleus (AGN) driven outflows can have a significant impact
on the evolution of the host galaxy. In this work, we compare the properties of
galaxies that hosts AGNs with and without outflows. Our sample consists of 103
AGNs identified by mid-IR color-color selection, and confirmed with optical
spectroscopy at a redshift range of 0.3 $\lesssim$ z $\lesssim$ 0.9. We fit the
[OIII] $\lambda$5007 line using spectra from the zCOSMOS survey to identify and
to study the occurrence of outflows. We find that ionized outflows are present
in $\sim$25\% of our sample, with the largest incidence at the highest [OIII]
and X-ray luminosity bins. The fastest outflows are found in the more extended
and massive galaxies. We do not observe a difference in the star formation rate
of AGNs with outflows compared to AGNs without outflows. From visual inspection
and non-parametric morphological studies, we obtain that outflows are
preferentially observed in galaxies with elliptical morphologies.
