  Recent arcsecond localizations of Fast Radio Bursts and identifications of
their host galaxies confirmed their extragalactic origin.While FRB 121102
resides in the bright region of a dwarf star forming galaxy, other FRBs reside
in more massive galaxies and are related to older stellar populations. We
compare the host galaxy properties of {nine} FRBs with those of several types
of stellar transients: from young to old population, long duration gamma ray
bursts (LGRBs), superluminous supernovae (SLSNe), Type Ib/Ic supernovae (SN
Ibc), Type II supernovae (SN II), type Ia supernovae (SN Ia), and short
duration gamma ray bursts (SGRBs). We find that as a whole sample, the stellar
mass and star formation rate of the FRB host galaxies prefer a medium to old
population, and are against a young population similar to LGRBs and SLSNe by a
null probability 0.02. Individually, the FRB 121102 host is consistent with
that of young population objects; the FRB 180924 environment is similar to that
of SGRBs; and the FRB 190523 environment is similar to those of SN Ia. These
results are consistent with the magnetar engine model for FRBs, if both
magnetars produced from extreme explosions (GRBs/SLSNe) and from regular
channels (e.g. those producing Galactic magnetars) can produce FRBs.
