  We present observations with the Advanced Camera for Surveys on the Hubble
Space Telescope of the nearby dwarf spheroidal galaxy KKH 22 = LEDA 2807114 in
the vicinity of the massive spiral galaxy IC 342. We derived its distance of
3.12+-0.19 Mpc using the tip of red giant branch (TRGB) method. We also used
the 6 m BTA spectroscopy to measure a heliocentric radial velocity of the
globular cluster in KKH22 to be +30+-10 km/s. The dSph galaxy KKH 22 has the
V-band absolute magnitude of -12.19 mag and the central surface brightness
mu_v,0 = 24.1 mag/sq.arcsec. Both the velocity and the distance of KKH 22 are
consistent with the dSph galaxy being gravitationally bound to IC 342. Another
nearby dIr galaxy, KKH 34, with a low heliocentric velocity of +106 km/s has
the TRGB distance of 7.28+-0.36 Mpc residing in the background with respect to
the IC 342 group. KKH 34 has a surprisingly high negative peculiar velocity of
-236+-26 km/s.
