Context. The Zone of Avoidance (ZoA) remains one of the last frontiers in constructing a comprehensive three-dimensional map of the Universe. Galactic extinction, stellar crowding, and confusion noise have historically limited the detection of background galaxies in these regions, with implications for large-scale structure and cosmological measurements. Aims. We assess the capability of the James Webb Space Telescope (JWST) Near Infrared Camera (NIRCam) to detect extragalactic sources in a heavily contaminated region of the Milky Way. Methods. We analyzed JWST/NIRCam wide-filter images of NGC 3324 with a customized implementation of SExtractor v2.28. Sources were detected in the F444W band, cross-matched with F090W and F200W, and validated against recent DAOPHOT point spread function photometry. A refined sample was obtained using full width at half maximum (FWHM)-signal-to-noise ratio criteria and visual inspection. Results. We identified 102 galaxies across the JWST/NIRCam field of view. The magnitude (F444W) distribution is bimodal, with similar to 10% brighter than m(F444W) < 15 mag and similar to 60% in the range 17 < m(F444W) < 19 mag. Typical sizes are FWHM approximate to 6.5 '', from compact to extended systems with isophotal areas of up to similar to 2000 pixels (similar to 7.9 arcsec(2)). Morphologies span from compact to spiral and lenticular systems, including a compact group at the eastern edge of the field. We also report the detection of transnebular galaxies, visible through the most opaque regions of the molecular cloud. Conclusions. These results demonstrate the potential of JWST/NIRCam to probe extragalactic sources through highly obscured Galactic regions, opening new avenues for mapping large-scale structures across the ZoA.