Spectral energy distribution for the accretion flow near the IMBH at the center of the stellar association calculated using a simple ADAF model with a numerical prescription described in Pesce et al. (2021). The input for the model is the time-averaged accretion rate extrapolated to the event horizon of the IMBH (Ṁ = 2.1 × 10⁻¹⁰ M_⊙ yr⁻¹) and the associated Eddington ratio (λ_Edd = 3.168 × 10⁻⁷). For comparison, we also show an SED for Sgr A* calculated with the same model using Ṁ = 2.1 × 10⁻⁸ M_⊙ yr⁻¹ and Eddington ratio λ_Edd = 2.258 × 10⁻⁷.