We report on the XMM-Newton observations of the BL Lac object MS 0737.9 + 7
841 during the performance verification phase. A simple power-law fit provi
des an adequate description of the integrated spectrum in the 0.2-10 keV en
ergy band. The photon index is slightly steeper in the EPIC pn data with Ga
mma = (2.38 +/- 0.01) compared to the EPIC MOS data (Gamma = (2.28 +/- 0.01
)). The difference is most probably due to the present uncertainties in the
calibration of the EPIC MOS and EPIC pn data sets. We report evidence for
intrinsic absorption in the distant BL Lac above the Galactic column (N-H,N
-Gal = 32 1020 cm(-2)) which is N-H,fit(z=0.315) = (2.70 +/- 0.20) 10(20) c
m(-2) in the EPIC pn data and N-H,fit(z=0.315) = (3.25 +/- 0.25) 10(20) cm(
-2) in the EPIC MOS data assuming neutral gas and solar abundances. The flu
x variations are found to be of the order of 10%. No significant spectral v
ariability is detected.