There exist constant radial surfaces, S, that may not be globally embeddable in R 3 for Kerr spacetimes with a > √ 3M/2. To compute the Brown and York (B-Y) quasi-local energy (QLE), one must isometrically embed S into R 3 . On the other hand, the Wang and Yau (W-Y) QLE embeds S into Minkowski space. In this paper, we examine the W-Y QLE for surfaces that may or may not be globally embeddable in R 3 . We show that their energy functional, E[τ ], has a critical point at τ = 0 for all constant radial surfaces in t = constant hypersurfaces using Boyer-Lindquist coordinates. For τ = 0, the W-Y QLE reduces to the B-Y QLE. To examine the W-Y QLE in these cases, we write the functional explicitly in terms of τ under the assumption that τ is only a function of θ. We then use a Fourier expansion of τ (θ) to explore the values of E[τ (θ)] in the space of coefficients. From our analysis, we discovered an open region of complex values for E[τ (θ)]. We also study the physical properties of the smallest real value of E[τ (θ)], which lies on the boundary separating real and complex energies.