  The analysis of a simultaneous XMM-Newton/BeppoSAX plus three previous
BeppoSAX observations revealed that NGC 7213 is a rather peculiar Seyfert 1. No
significant Compton reflection component was observed, while an iron line
complex, best explained in terms of three narrow lines, is clearly apparent in
the data. Due to the absence of the reflection component, the neutral iron line
is likely not produced in a Compton-thick material, but current data do not
allow to choose between a Compton-thin torus and the BLR. The two ionized iron
lines from \ion{Fe}{xxv} and \ion{Fe}{xxvi} may be produced in a photoionized
gas with a column density of a few 10$^{23}$ cm$^{-2}$, in analogy with the
case of NGC 5506.
