This galaxy presents as an edge-on spiral, exhibiting a prominent and somewhat elongated central bulge. The bulge displays a yellowish hue, possibly indicating an older stellar population. A faint dust lane is visible bisecting the galaxy, indicative of a significant disk component. The spiral arms are tightly wound and appear relatively smooth with some blueish regions, which suggests regions of recent star formation. There is no evidence of a major merger or significant tidal disturbance. The general morphology suggests a relatively undisturbed spiral galaxy, seen at a high inclination.
