  We present the results of an ASCA observation of the low-luminosity Seyfert
1.5 galaxy NGC 5033. A point-like X-ray source with a luminosity of 2.3x10^{41}
erg s^{-1} in the 2--10 keV band (at 18.7 Mpc; Tully 1988, AAA045.002.054) was
detected at the nucleus. The X-ray light curve shows variability on a timescale
of ~10^4 s with an amplitude of ~20%. The X-ray continuum is represented by a
weakly absorbed (N_H~9x10^{20} {cm^{-2}) power-law with a photon index of
1.72+/-0.04, which is quite similar to Seyfert 1 galaxies with higher
luminosities. A Fe Kalpha emission line is detected at 6.40^{+0.08}_{-0.06} keV
(redshift corrected) and the equivalent width is 290+/-100 eV. The line width
is unresolved. The narrower line width and larger equivalent width compared to
Seyfert 1s imply that fluorescent Fe Kalpha emission from matter further out
from the center than the accretion disk significantly contributes to the
observed Fe Kalpha line. We suggest that fluorescent Fe Kalpha emission from
the putative torus contributes to the observed Fe Kalpha line.
