The galaxy exhibits a prominent, relatively bright central bulge. Faint spiral arm structures are visible emanating from the central region. The spiral arms appear somewhat tightly wound and not very well-defined. There is a moderate amount of galactic disk, which appears patchy and irregular. The colouration of the galaxy suggests ongoing star formation, with regions of bluer light scattered along the spiral arms, contrasting with the yellowish hue of the bulge. Evidence indicates there could be a slight disturbance from a minor merging event.