NGC 4314 (top row) is an (R)SB(rl,nr)a galaxy (Buta et al., in prep.) with a passive inner ring-lens. NGC 1672 (bottom row) is an (R′)SA(rs,nr)b galaxy (Buta et al., in prep.) whose inner pseudoring is still forming stars. In the first case the inner feature does not emit in the FUV and Hα. There is a significant amount of emission in these bands for the active inner feature. The prominent ring feature in NGC 4314 is a nuclear ring. The 3.6   μm images are from the S⁴G, the FUV images come from GALEX’s NGS survey, and the Hα images come from Knapen et al. (2004) and the HLA.