The galaxy presents as a spiral galaxy with two well-defined spiral arms. These spiral arms are not tightly wound, displaying a more open morphology. There is a small central bulge. A bar structure also appears to run through the bulge of the galaxy. There is some level of blueness associated with the spiral arms suggesting the presence of more recent star formation. The galaxy displays no signs of tidal disruption or ongoing major merger events, however, there are some signs of disturbances in the spiral arm morphology.
