The galaxy presents as a spiral galaxy. It exhibits a moderate central bulge, appearing less concentrated and more diffused. The spiral arms are quite prominent and moderately wound, suggesting an intermediate stage in the galaxy's evolution. The morphology is dominated by the presence of these spiral arms, which appear somewhat patchy. While the majority of the galaxy appears undisturbed, there is a hint of a minor disturbance that may be due to a small interaction or possible merger. A weak bar structure bisects the central bulge. The overall structure implies ongoing, but not exceptionally vigorous, star formation.