In the present work we report the Bep-poSAXserendipitous discovery of the t
ype 2 AGN 1SAXJ2234.8-2541 in the MECS field of view when pointing at the S
eyfert 2 galaxy NGC7314. The source is optical identified with the bright (
m(B)=14.40) galaxy ESO533-G50 at redshift z=0.026. The source is clearly de
tected at energies above 4 keV but barely visible below this energy implyin
g heavy obscuration intrinsic to the source. Spectral analysis indicates a
column density of the order of 2-3 x 10(23) cm(-2) and a power law photon i
ndex compatible with values often seen in active galaxies. These X-ray char
acteristics suggest a Seyfert 2 classification for 1SAXJ2234.8-2541. Subseq
uent spectroscopy of the optical counterpart, ESO533-G50, performed with th
e ESO 1.52m telescope at La Silla Observatory, confirms the type 2 nature o
f this source and therefore its identification with the X-ray source. We al
so report the marginal detection of an iron line centered at 7.29 +/- 0.47
keV and having an equivalent width of 46(-398)(+636), eV; although marginal
, this result is indicative of the presence of warm material in the source.
If instead the line is associated to cold material, we estimate an upper l
imit to its equivalent width of 290 eV. The overall characteristics of 1SAX
J2233.8-2541 strongly suggest that the sourer is Compton thin.