The galaxy presents as a relatively face-on spiral. Two prominent spiral arms are visible, extending from a central bulge. The arms appear loosely wound, displaying considerable star formation activity evidenced by their patchy and clumpy appearance. There may be faint signs of additional spiral structure but the limitations of image clarity make it difficult to be sure. There is no obvious indication of a bar structure, and there are no significant signs of tidal disturbance or ongoing major merger activity with a companion galaxy, although some minor irregularities are apparent. The central bulge appears relatively small and does not dominate the overall luminosity of the galaxy.
