The galaxy presents as a spiral, observed at an angle neither fully face-on nor edge-on. The central bulge appears relatively small and exhibits a yellowish hue, suggestive of an older stellar population. Faint spiral arms extend outwards. The arms are tightly wound close to the bulge and open up a bit further out. The disc is mostly smooth, but there is a small amount of disturbance. The blueish tint indicates the presence of ongoing star formation within these arms. This galaxy appears relatively isolated, showing no signs of interaction with other galaxies.
