The asymptotic symmetry analysis of Maxwell theory at spatial infinity of Minkowski space with d ≥ 3 is performed. We revisit the action principle in de Sitter slicing and make it well-defined by an asymptotic gauge fixing. In consequence, the conserved charges are inferred directly by manipulating surface terms of the action. Remarkably, the antipodal condition on de Sitter space is imposed by demanding regularity of field strength at light cone for d ≥ 4. We also show how this condition reproduces and generalizes the parity conditions for inertial observers treated in 3+1 formulations. The expression of the charge for two limiting cases is discussed: Null infinity and inertial Minkowski observers. For the separately-treated 3d theory, a set of non-logarithmic boundary conditions at null infinity are derived by large boost limit.Recent interest in ASG of Maxwell theory in flat space emanated from the discovery that soft photon theorem in QED is the Ward identity of the asymptotic symmetry group [7,8]. Concerned with that motivation, research on asymptotic symmetries is mostly performed in null slicing (Bondi coordinates) of flat space, where the surface of integration is (almost) lightlike-separated from the scattering event [7,[9][10][11][12][13][14]. The charges "at null infinity" have also been generalized to subleading orders [15][16][17].The asymptotic symmetry group of Maxwell theory at spatial infinity is, as far as we know, restricted to three and four dimensions [15,[18][19][20][21]. Spatial infinity examination allows applying the canonical methods and define the ASG in a standard way. In [15], the multipole moments of a static configuration were exhibited as asymptotic symmetry charges. In [19], the charges were defined in de Sitter slicing of flat space (explained later), and the null infinity charges would be recovered if the integration surface approached null infinity. We will follow much similar path in this paper, recovering [12,22] at null infinity.