The galaxy presents as a disk-dominated spiral galaxy, seen at a slight angle from edge-on. A prominent central bulge exhibits a smooth, yellowish-white color, indicating an older stellar population. Strong bar structure is observed through the bulge. The disk shows well-defined spiral arms originating from the ends of the bar. The arms appear tightly wound and traced by regions of bluer light, suggesting active star formation. A minor disturbance in the morphology of the arms, possibly indicating a gravitational interaction, is suspected.
