The galaxy presents as an edge-on spiral with a clear disk component. The central bulge appears relatively prominent and elongated along the major axis of the disk and exhibits a smooth, rounded morphology. The disk is thin and exhibits a noticeable warp. Dust lanes are faintly visible within the disk, tracing the spiral structure and contributing to the redder coloration near the mid-plane. There is evidence of active star formation within the galaxy, as indicated by the blueish hue of the galaxy. There appears to be no sign of any major merging events, but some minor disturbances may be present. The galaxy exhibits a moderate level of star formation activity.
