This galaxy appears to be a spiral galaxy viewed at a moderate inclination. It exhibits a prominent central bulge that is roughly 1/3 the size of the galactic disk. The spiral arms are well-defined and display a predominantly two-arm structure. The arms are somewhat tightly wound closest to the bulge and open as you move further out into the disk. The disk itself appears to be slightly disturbed, possibly indicative of minor interactions or internal dynamics. The galaxy displays evidence of active star formation within its spiral arms, with noticeable blue regions indicating the presence of young, hot stars. There is no bar visible.
