Comparison between the properties of the MaNGA galaxy M-8341-09101 and the Milky Way. Panel a: comparison between the radial oxygen abundance distributions. The blue circles denote the T_e-based abundances in individual H II regions in the MW (comes from panel b of Fig. 2) and the solid line is the best fit to those data. The grey points are the R calibration-based abundances in the spaxels of M-8341-09101 and the dashed line is the linear fit to those data points. Panel b: comparison between rotation curves. The points denote the rotation curve of the Milky Way from Eilers et al. (2019). The rotation curve of M-8341-09101 is shown by the line.