The galaxy presents as a barred spiral system, exhibiting a disk-like structure. The central bulge appears small and diffuse, with a yellowish-white hue indicating an older stellar population. Tightly wound spiral arms extend from the ends of the central bar. The arms are relatively smooth and appear to have a high concentration of older stars. Patches of blue light are visible within the spiral arms, likely indicating regions of active star formation. The dust lanes are somewhat visible, but lack a clear presence. Overall, the galaxy's disk is tilted from our line of sight.
