Spectral energy distribution of NGC 1487. The plot displays total intensity data with different observations: GLEAM-X data (Ross et al. 2024), RACS-Low data (McConnell et al. 2020), ASKAP EMU main survey (Hopkins et al. 2025), MeerKAT 1.28 GHz data, ATCA L/S-band, C-band, and X-band data presented in this work, and further data from the work of Grundy et al. (2025). We show the best-fit in red with 1σ uncertainty sampled by EMCEE. The blue, orange, and green dotted lines represent the different components of the best-fit model.