The galaxy presents as a spiral type, exhibiting prominent spiral arm structures. These arms are somewhat loosely wound and appear patchy, with varying degrees of luminosity along their lengths. There is evidence of ongoing star formation within the arms, indicated by the presence of bluer regions.

A central bulge is visible, though it appears relatively small in proportion to the overall size of the galaxy. The bulge exhibits a smoother texture and a yellowish-white color, suggesting an older stellar population. A faint bar structure may exist, as there seems to be a slightly elongated region of increased brightness running through the central bulge.

The disk component of the galaxy is significant, contributing substantially to the overall luminosity. The galaxy appears relatively face-on, and it does not exhibit any signs of significant tidal disruption or interaction with other galaxies.
