The galaxy presents as a spiral type, exhibiting a disk-like structure. The arms are distinctly visible, tracing a clear spiral pattern from the central bulge. It appears to be a barred spiral galaxy, with a prominent bar-like structure extending across the central region. The spiral arms are moderately wound. There appears to be a significant amount of ongoing star formation. The bulge exhibits a moderate size. There are two very distinct arms. No major merging disturbances are apparent in the galaxy's morphology.
