The observed galaxy exhibits a distinct spiral structure. The spiral arms are prominent, displaying a relatively tightly wound morphology. Two main spiral arms are visible. The galaxy possesses a noticeable bulge component, which appears of moderate size relative to the overall galactic disk. There is some evidence of a weak bar structure spanning the central region of the galaxy. The galaxy's disk is not viewed edge-on. The overall appearance suggests a relatively undisturbed structure with no clear indications of significant recent or ongoing merger activity.
