  We present a spectropolarimetric analysis of the hot star V352Peg. We have
acquired 18 spectropolarimetric observations of the star with ESPaDOnS at the
CFHT between 2018 and 2019 and completed our dataset with one archival ESPaDOnS
measurement obtained in 2011. Our analysis of the spectra shows that the star
is on the main sequence and chemically peculiar, i.e. it is a Bp star, with
overabundances of iron peak elements (Ti, Cr and Fe) and underabundance of He
and O. Through a Least-Square Deconvolution of each spectrum, we extracted the
mean Zeeman signature and mean line profile of thousands of spectral lines and
detected a magnetic field in V352Peg. By modelling the Stokes I and V profiles
and using the Oblique Rotator Model, we determined the geometrical
configuration of V352Peg. We also performed Zeeman-Doppler Imaging (ZDI) to
provide a more detailed characterization of the magnetic field of V352Peg and
its surface chemical distributions. We find a magnetic field that is mainly
dipolar, dominantly poloidal, and largely non-axisymmetric with a dipole field
strength of $\sim$9 kG and a magnetic axis almost perpendicular to the rotation
axis. The strong variability of Stokes I profiles also suggests the presence of
chemical spots at the stellar surface.
