Result of two-component spectro-photometric modeling of the spatial bin at R = +18 ± 3″. Middle and top panels: spectrum (black) and best-fit spectral model (red). Two stellar components of the model are shown in blue and green colors. Orange lines highlight the emission-line model. Residuals are presented in the mid panel in gray bordered by the error level (black lines). Bottom panel: SED part of the model. Observed magnitudes are shown in large black circles, and the best-fit SED model is shown with red crosses. Blue and green circles correspond to SED models of individual components whose low-resolution spectra are shown by colored lines.