The galaxy presents a clear spiral morphology, exhibiting well-defined arms that emanate from a central bulge. The bulge appears yellowish, suggesting an older stellar population. The spiral arms show a bluish hue, indicative of ongoing star formation. These arms appear moderately tightly wound around the central bulge. The spiral arms appear to be comprised of multiple arms. There appears to be evidence of a bar structure running through the central region of the galaxy. There is no immediately apparent evidence of major mergers or significant disturbances in the galaxy's overall structure, though minor disturbances cannot be ruled out. The galaxy is not observed edge-on, and is well-resolved.
