Extremal black holes of four dimensional N = 1 supergravity coupled to vector and chiral multiplets can be viewed as solitonic solutions of the theory. In this paper, we particularly study a static spherical symmetric black holes. In the asymptotic region the complex scalars are frozen which can be viewed as the critical points of the black hole and the scalar potentials with vanishing scalar charges. then, it turns out that the asymptotic geometries have a constant scalar curvature which in general are not Einstein. These spaces are boundaries of the black holes which could also correspond to the near horizon geometries if the value of the scalars in both regions coincides.
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