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We present radio continuum mapping, optical imaging and spectroscopy of thenewly discovered double-peaked broad-lined AGN WISE J233237.05-505643.5 atredshift z = 0.3447. This source exhibits an FR-I and FR-II hybrid-morphology,characterized by bright core, jet, and Doppler-boosted lobe structures in ATCAcontinuum maps at 1.5, 5.6, and 9 GHz. Unlike most FR-II objects, W2332-5056 ishosted by a disk-like galaxy. The core has a projected 5" linear radio featurethat is perpendicular to the curved primary jet, hinting at unusual and complexactivity within the inner 25 kpc. The multi-epoch optical-near-IR photometricmeasurements indicate significant variability over a 3-20 year baseline fromthe AGN component. Gemini-South optical data shows an unusual double-peakedemission-line features: the centroids of the broad-lined components of H-alphaand H-beta are blueshifted with respect to the narrow lines and host galaxy by~ 3800 km/s. We examine possible cases which involve single or doublesupermassive black holes in the system, and discuss required futureinvestigations to disentangle the mystery nature of this system.

WISE J233237.05-505643.5: a Double-Peaked Broad-Lined AGN with Spiral-Shaped Radio Morphology