In this work, we will study the boundary behaviors of a spacelike positive constant mean curvature surface (Sigma ) in the Schwarzschild spacetime exterior to the black hole. We consider two boundaries: the future null infinity (mathcal {I}^+) and the horizon. Suppose near (mathcal {I}^+), (Sigma ) is the graph of a function (-P(textbf{y},s)) in the form (overline{v}=-P), where (overline{v}) is the retarded null coordinate with (s=r^{-1}) and (textbf{y}in mathbb {S}^2). Suppose the boundary value of (P(textbf{y},s)) at (s=0) is a smooth function f on the unit sphere (mathbb {S}^2). If P is (C^4) at (mathcal {I}^+), then f must satisfy a fourth order PDE on (mathbb {S}^2). If P is (C^3), then all the derivatives of P up to order three can be expressed in terms of f and its derivatives on (mathbb {S}^2). For the extrinsic geometry of (Sigma ), under certain conditions we obtain decay rate of the trace-free part of the second fundamental forms (mathring{A}). In case (mathring{A}) decays fast enough, some further restrictions on f are given. For the intrinsic geometry, we show that under certain conditions, (Sigma ) is asymptotically hyperbolic in the sense of Chruściel–Herzlich (Pac J Math 212(2):231–264, 2003). Near the horizon, we prove that under certain conditions, (Sigma ) can be expressed as the graph of a function u which is smooth in (eta =left( 1-frac{2m}{r}right) ^{frac{1}{2}}) and (textbf{y}in mathbb {S}^2), and all its derivatives are determined by the boundary value u at (eta =0). In particular, a Neumann-type condition is obtained. This may be related to a remark of Bartnik (in: Proc Centre Math Anal Austral Nat Univ, 1987). As for intrinsic geometry, we show that under certain conditions the inner boundary of (Sigma ) given by (eta =0) is totally geodesic.