SED of NGC 4593 derived using the CIGALE software. The plot shows the observed SED, indicated by red points, compared to the best-fit model represented by the solid black line. The constituent components of the model are illustrated as follows: dust emission (red line), AGN emission (orange line), and stellar emission, both attenuated (yellow dashed line) and unattenuated (blue dashed line). The vertical axis denotes the flux density S​_ν in mJy, while the horizontal axis represents the wavelength λ in μm. This SED plot provides a comprehensive view of the various emission components contributing to the observed radiation from NGC 4593.