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We present observations with the Advanced Camera for Surveys on the HubbleSpace Telescope of the nearby dwarf spheroidal galaxy KKH 22 = LEDA 2807114 inthe vicinity of the massive spiral galaxy IC 342. We derived its distance of3.12+-0.19 Mpc using the tip of red giant branch (TRGB) method. We also usedthe 6 m BTA spectroscopy to measure a heliocentric radial velocity of theglobular cluster in KKH22 to be +30+-10 km/s. The dSph galaxy KKH 22 has theV-band absolute magnitude of -12.19 mag and the central surface brightnessmu_v,0 = 24.1 mag/sq.arcsec. Both the velocity and the distance of KKH 22 areconsistent with the dSph galaxy being gravitationally bound to IC 342. Anothernearby dIr galaxy, KKH 34, with a low heliocentric velocity of +106 km/s hasthe TRGB distance of 7.28+-0.36 Mpc residing in the background with respect tothe IC 342 group. KKH 34 has a surprisingly high negative peculiar velocity of-236+-26 km/s.

KKH 22, the first dwarf spheroidal satellite of IC 342