The galaxy presents as a spiral galaxy with a significant disk component. The spiral arms are prominent, with an estimated two main arms visible. These arms exhibit a grand design, with a loose winding pattern extending outward from the central bulge. There are no signs of flocculent arms. The central bulge appears moderate in size, possibly housing a bar structure, though it is not highly defined. The inclination of the galaxy is relatively edge-on, though the angle of the disk is not fully aligned with our line of sight. There is an indication of possible minor disturbances from gravitational interactions with a companion galaxy, however no complete merging is visible.
