The galaxy presents as a spiral with a notable disk structure. Spiral arms are visible, though somewhat diffuse. They appear relatively tightly wound. The central bulge is prominent, exhibiting a concentrated luminosity, which is roughly orange in color. The disk shows a bluer hue, consistent with regions of younger, hotter stars. The galaxy's overall orientation appears close to face-on. There may be a weak bar feature present. The morphology appears relatively undisturbed, showing no strong signs of recent or ongoing major merger events.
