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Age-related changes in the radiologic findings of lobular endocervical glandular hyperplasia: a multicenter study

Jpn J Radiol. 2025 Feb 14. doi: 10.1007/s11604-025-01748-y. Online ahead of print.

ABSTRACT

PURPOSE: To investigate the age-related changes in magnetic resonance imaging (MRI) findings of lobular endocervical glandular hyperplasia (LEGH) during long-term follow-up.

MATERIALS AND METHODS: This multicenter study included 91 patients who underwent preoperative MRI and had a histopathological diagnosis of LEGH, atypical LEGH, or adenocarcinoma in situ (AIS) with LEGH after surgical resection. Thirty patients underwent follow-up MRIs at intervals of more than 3 months. According to the age and menopausal status, patients were categorized into four groups: group A, 31-40 years; group B, 41-50 years (premenopausal); group C, more than 50 years (premenopausal); group D, postmenopausal. Differences in the MRI findings (size and morphological pattern) were compared among the four groups.

RESULTS: The lesion volume was the largest in group C and smallest in group D, showing a statistically significant difference (p < 0.05). The typical cosmos pattern was seen in 60.0% of group A, 62.2% of group B, 75.0% of group C, and 29.2% of group D. The cosmos pattern was significantly less frequent in postmenopausal patients compared to premenopausal patients (p < 0.05). During follow-up, five of 12 individuals in group A exhibited the typical cosmos pattern. Among the seven individuals who did not initially show the cosmos pattern, two later developed the typical cosmos pattern. No changes in the lesion pattern were observed in participants in their 40 s up to the premenopausal 50 s. From the premenopausal 50 s to the postmenopausal period, the cosmos pattern changed to a microcystic pattern in one case of atypical LEGH.

CONCLUSIONS: LEGH increases in volume with age until menopause, along with an increasing frequency of the typical cosmos pattern in MRI. However, after menopause, both the volume of the lesion and frequency of the typical cosmos pattern decrease.

PMID:39951245 | DOI:10.1007/s11604-025-01748-y

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