This galaxy exhibits a distinct spiral structure, with tightly wound arms emanating from a prominent central bulge. The bulge appears moderately sized, contributing significantly to the overall luminosity of the galaxy. A bar-like structure appears to cut through the center of the galaxy. The spiral arms are well-defined and show evidence of active star formation, indicated by their slightly bluer color. The galaxy is not viewed perfectly face-on, presenting a slight inclination. The disk of the galaxy shows minimal evidence of major disturbances or ongoing merging events.
