The unified description of gauge and Higgs fields based on non-commuta
tive geometry due to Connes has a similar structure to Kaluza-Klein th
eory, though it is a 4-dimensional theory. Its extension to a theory i
n curved spacetime is, then, expected to give a Brans-Dicke type gravi
ty in which Higgs-like scalar fields couple to the gravitational field
. In this paper, we study a B-D type gravity using the matrix coordina
te method originated by Coquereaux. In particular, the introduction of
two kinds of scalar fields is discussed in detail from the viewpoint
of cosmology.