Velocity ellipses for the quasi-axisymmetric orthogonal NSD model, constructed from stars in the region |ℓ| < 0.9° and |b| < 0.25°. Left: all stars show l_v ≈ −89.5° and low anisotropy (β = 0.22), appearing nearly axisymmetric due to contamination from older large-scale bar stars. Right: result when selecting younger stars (τ_⋆ < 5 Gyr) that predominantly trace the late-forming NSD yields l_v≈79.2° with higher anisotropy β = 0.62. This demonstrates that an orthogonal NSD can produce positive l_v, similar to a nuclear bar with its near side at negative longitudes.