  We compare the photometric properties and specific star formation rate (sSFR)
of classical and pseudo-bulge galaxies with $M_* \ge 10^{9.5} \rm M_{\odot}$ at
$0.5\le z<1.0$, selected from all five CANDELS fields. We also compare these
properties of bulge galaxies at lower redshift selected from MaNGA survey (Hu
et al. 2024). This paper aims to study the properties of galaxies with
classical and pseudo-bulges at intermediate redshift, to compare the
differences between different bulge types, and to understand the evolution of
bulges with redshift. Galaxies are classified into classical bulge and
pseudo-bulge samples according to the S$\mathrm{\acute{e}}$rsic index n of the
bulge component based on results of two-component decomposition of galaxies, as
well as the position of bulges on the Kormendy diagram. For the 105 classical
bulge and 86 pseudo-bulge galaxies selected, we compare their size, luminosity,
and sSFR of various components. At given stellar mass, most classical bulge
galaxies have smaller effective radii, larger $B/T$, brighter and relatively
larger bulges, and less active star formation than pseudo-bulge galaxies.
Besides, the two types of galaxies have larger differences in sSFR at large
radii than at the central region at both low and mid-redshifts. The differences
between properties of the two types of bulge galaxies are in general smaller at
mid-redshift than at low redshift, indicating that they are evolving to more
distinct populations towards the local universe. Bulge type is correlated with
the properties of their outer disks, and the correlation is already present at
redshift as high as $0.5<z<1$.
