This galaxy presents a clear spiral structure, exhibiting multiple arms that are tightly wound around a central bulge. The bulge appears moderately sized and is yellowish, indicating an older stellar population. The spiral arms are well-defined and exhibit a bluer hue, suggesting active star formation. Patches of differing color along the arms indicate clusters of new stars. There is a slight distortion in the outer arms of the galaxy, suggesting a possible gravitational interaction with a neighboring galaxy or a previous merger event. There may be a weak bar-like structure in the center of the galaxy. The galaxy is not perfectly face-on, tilted slightly relative to our line of sight. Overall, the galaxy seems relatively undisturbed, aside from possible past interactions, showing a spiral morphology with a distinct bulge and tightly wound arms.
