Assessing Facial Asymmetry in Postoperative Patients With Unilateral Coronal Craniosynostosis

Despite surgical correction of unilateral craniosynostosis (ULC), complex cranial base angulation can result in partial reversion to preoperative deformity with growth and time. Using 3-dimensional imaging, dysmorphic facial features of ULC in school-age patients were quantified and related to how they contribute to overall facial asymmetry and patient-reported outcomes.

Children who underwent surgical correction of ULC were recruited from Yale University and Children's Hospital of Philadelphia. The 3D photographs were analyzed utilizing a Procrustes analysis of shape. Pearson's correlation was used to determine dysmorphic features' impact on overall asymmetry. Patients were stratified into "moderate" and "severe" asymmetry. Finally, asymmetry was correlated to patient-reported outcome scores. Statistical analysis was performed with SPSS-25 with P < 0.05 as statistically significant.

Twenty-one patients were included with average age at analysis of 12.3 years. Fifty-seven percent of patients had right-sided fusion. The overall Procrustes analysis indicated a root mean square difference of 2.21 mm. Pearson's correlation indicated that the facial middle 3rd (P ≤ 0.001), orbital dystopia (P < 0.001), chin point deviation (P = 0.011), and nasal root angulation (P = 0.019) contributed most to overall asymmetry. Patients in the severe asymmetry cohort had greater facial middle-third asymmetry (P < 0.001) and orbital dystopia (P < 0.001). Asymmetry did not correlate with patient-reported outcomes.

Patients with ULC have persistent facial asymmetry at school-age with the greatest levels of asymmetry in the facial middle-third, orbit, and nasal root. Beyond the cranial dysmorphology, initial skull base angulation in unilateral coronal craniosynostosis manifests in long-term mid and lower-third facial asymmetry.