| Summary: | We present high-resolution radio interferometric imaging observations of the radio source NVSS J182659+343113 (hereafter J1826+3431), the proposed radio counterpart of the <inline-formula><math display="inline"><semantics><mi>γ</mi></semantics></math></inline-formula>-ray source, 3EG J1824+3441 detected by the Energetic Gamma Ray Experiment Telescope (EGRET) on board the <i>Compton Gamma Ray Observatory</i> satellite. We analyzed eight epochs of archival multi-frequency very long baseline interferometry data. We imaged the asymmetric core–jet structure of the source, and detected apparent superluminal motion in the jet. At the highest observing frequency, <inline-formula><math display="inline"><semantics><mrow><mn>15.3</mn></mrow></semantics></math></inline-formula> GHz, the core shows high brightness temperature indicating Doppler boosting. Additionally, the radio features undergo substantial flux density variability. These findings strengthen the previous claim of the association of the blazar J1826+3431 with the possible <inline-formula><math display="inline"><semantics><mi>γ</mi></semantics></math></inline-formula>-ray source, 3EG J1824+3441.
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