Distribution of the PA misalignment between mass and light, and the local galaxy density, Σ₁₀, and its variations. Left: Variations of Σ₁₀ are based on different galaxy selection criteria, including the number of galaxies considered and flux-based thresholds. Right: Variations correspond to different weighting schemes used in defining Σ₁₀ (i.e., definitions B, C, and D). Systems with low ellipticity (q_L>0.9) are excluded from both cases. While the baseline definitions, Σ₁₀ and Σ₂₀, exhibit a moderate to strong correlation with the PA misalignment, other definitions show only weak to very weak correlations. Therefore, we cannot robustly conclude a strong relationship between PA misalignment and local galaxy density.