Postage stamps of the edge-on galaxy UVCANDELS 20524 show that while the F160W image is bulge-dominated, the F275W image is bright mainly in the outskirts—especially the upper left—rather than the center. This is consistent with dust obscuration, as supported by the A_V map. However, the UV-bright region in the lower right does not show elevated properties, including A_V, ruling out dust obscuration there. The SFR and stellar mass density maps show enhanced values along the top edge of the disk. The t₅₀ map reveals both older- and younger-than-average regions in this area. Overall, these features may result from projection effects in an edge-on galaxy.