  We present medium deep CCD imaging in B, V, and I of the Pegasus Dwarf galaxy
(And VI) which was recently found by Karachentsev & Karachentseva (1998), and
independently also by Armandroff et al. (1999). The Calar Alto 2.2m images show
a low surface brightness galaxy. Its structure resembles that of the other
known dSph companions of M31 And I, II, III, and V. The brightest stars are
resolved in all three colors. Color-magnitude diagrams in either B-V or V-I
show the tip of the red giant branch which allows us to estimate a true
distance modulus of $24.5 \pm 0.2$. The color-magnitude diagrams and the
structure show no evidence for recent star formation, thus, a classification as
spheroidal dwarf galaxy with a rather old population seems appropriate. The
total absolute magnitude of this dwarf is $M_{V,0} = -10.4\pm0.2$.
