Abstract
ABSTRACTShiga toxin-producing Escherichia coli (STEC) O26 is the predominant non-O157 serogroup causing hemolytic uremic syndrome worldwide. Moreover, the serogroup is highly dynamic and harbors several pathogenic clones. Here, we investigated the phylogenetic relationship of STEC O26 at a global level based on 1,367 strains from 20 countries deposited in NCBI and Enterobase databases. The whole-genome-based analysis identified a new genetic clade, called ST29C4. The new clade was unique in terms of multilocus sequence type (ST29), CRISPR (group Ia), and dominant plasmid gene profile (ehxA+/katP-/espP-/etpD-). Moreover, the combination of multiple typing methods (core genome single nucleotide polymorphism [SNP] typing, CRISPR typing, and virulence genes analysis) demonstrated that this new lineage ST29C4 was in the intermediate phylogenetic position between ST29C3 and other non-ST29C3 strains. Besides, we observed that ST29C4 harbored extraintestinal pathogenic E. coli (ExPEC)-related virulence gene (VG), tsh, and STEC-associated VG, stx2a, suggesting the emergence of a hybrid pathogen. The ST29C4 strains also exhibited high similarity in stx2a-prophage and integrase with the O104:H4 strain, further demonstrating its potential risk to human health. Collectively, the large-scale phylogenetic analysis extends the understanding of the clonal structure of O26 strains and provides new insights for O26 strain microevolution.IMPORTANCE Shiga toxin-producing Escherichia coli (STEC) O26 is the second prevalent STEC serogroup only to O157, which can cause a series of diseases ranging from mild diarrhea to life-threatening hemolytic uremic syndrome (HUS). The serogroup is highly diverse and multiple clones are characterized, including ST29C1-C3 and ST21C1-C2. However, the phylogenetic relationship of these clones remains fully unclear. In this study, we revealed a new genetic clade among O26 strains, ST29C4, which was unique in terms of CRISPR, multilocus sequence type (MLST), and plasmid gene profile (PGP). Moreover, the combination of multiple typing methods demonstrated that this new clone was located in the intermediate phylogenetic position between ST29C3 and other non-ST29C3 strains (i.e., ST29C1-C2 and ST21C1-C2). Overall, the large-scale phylogenetic analysis extends our current understanding of O26 microevolution.
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