  We present HST WFPC2 and ground-based images of the low surface brightness
dwarf Irr/Sph galaxy KKR~25 in Draco. Its colour-magnitude diagram shows red
giant branch stars with the tip at I = 22.32 mag, and the presence of some blue
stars. The derived true distance modulus, 26.35 \+- 0.14 mag, corresponds to
linear distances of KKR25 from the Milky Way and from the Local Group centroid
of 1.86 and 1.79 Mpc, respectively. The absolute magnitude of the galaxy, M_V =
-10.48, its linear diameter (0.54 Kpc) and central surface brightness (24.0 +-
0.2 mag\arcsec^2) are typical of other dIrr/dSphs in the Local Group. Being
situated just beyond the radius of the zero-velocity surface of the Local
Group, KKR25 moves away from the LG centroid at a velocity of V_{LG} = + 72
km/s.
