It is a Be star; a rapidly rotating star that is hosting a circumstellar disk of hot, decreted gas. It is a photometrically variable Be star, having a brightness that ranges from 4.4 down to 4.51 in visual magnitude, and has been classified as a Gamma Cassiopeiae variable.
It is a Be star; characterized by rapid rotation and hosting a circumstellar disk of hot, condensed gas. It exhibits photometric variability with brightness ranging from 4.4 to 4.51 in visual magnitude, and falls under the Gamma Cassiopeiae variable classification.