This galaxy exhibits a clear spiral structure. The spiral arms are tightly wound around a prominent central bulge, which appears quite luminous and concentrated. The color suggests a significant population of older stars within the bulge. The spiral arms themselves show variations in color and brightness, hinting at ongoing star formation regions interspersed with older stellar populations. The galaxy is not perfectly symmetrical, with some irregularities in the arm structure, possibly indicating gravitational interactions or minor disturbances. There is no obvious sign of a strong bar feature across the center of the galaxy. The overall appearance is consistent with that of a relatively massive spiral galaxy with a moderate-sized bulge and a mixture of young and old stellar populations.
