  We present an XMM-Newton observation of the Seyfert-LINER galaxy NGC 7213.
The RGS soft X-ray spectrum is well fitted with a power law plus soft X-ray
collisionally ionised thermal plasma (kT = 0.18 +0.03/-0.01 keV). We confirm
the presence of Fe I, XXV and XXVI K-alpha emission in the EPIC spectrum and
set tighter constraints on their equivalent widths of 82 +10/-13, 24 +9/-11 and
24 +10/-13 eV respectively. We compare the observed properties together with
the inferred mass accretion rate of NGC 7213, to those of other Seyfert and
LINER galaxies. We find that NGC 7213 has intermediate X-ray spectral
properties lying between those of the weak AGN found in the LINER M81 and
higher luminosity Seyfert galaxies. There appears to be a continuous sequence
of X-ray properties from the Galactic Centre through LINER galaxies to
Seyferts, likely determined by the amount of material available for accretion
in the central regions.
