  We use near-infrared (NIR) spectroscopy covering simultaneously the $zJHK$
bands to look for outflowing gas from the nuclear environment of 1H0707-495
taking advantage that this region is dominated by low-ionization broad line
region (BLR) lines, most of them isolated. We detect broad components in HI,
FeII and OI, at rest to the systemic velocity, displaying full width at half
maximum (FWHM) values of ~500 km s$^{-1}$, consistent with its classification
as a narrow-line Seyfert~1 AGN. Moreover, most lines display a conspicuous
blue-asymmetric profile, modeled using a blueshifted component, whose velocity
shift reaches up to ~826 km s$^{-1}$. This last feature can be interpreted in
terms of outflowing gas already observed in X-ray and UV lines in 1H0707-495
but not detected before in the low-ionization lines. We discuss the relevance
of our findings within the framework of the wind scenario already proposed for
this source and suggest that the wind extends well into the narrow line region
due to the observation of a blueshifted component in the forbidden line of
[SIII] $\lambda$9531.
