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 re
d giant branch stars with the tip at I = 22.(m)32, and the presence of some
blue stars. The derived true distance modulus, 26.(m) 35 +/- 0.(m)14, corr
esponds to linear distances of KKR 25 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 surf
ace brightness (Sigma (0,V) = 24.(m) 0 +/- 0.(m) 2/square") 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, KKR 25 moves away from the
LG centroid at a velocity of V-LG = +72 km s(-1).