The galaxy presents a disk-like morphology with notable spiral arm structure. The arms appear relatively tightly wound. A central bulge is apparent, transitioning smoothly into the disk. The galaxy exhibits a moderate degree of ellipticity. Dust lanes are visible within the spiral arms, particularly on the periphery of the bulge. The color distribution suggests a mix of stellar populations, with a central region that shows a bluer hue. There is no evidence of any major merging events.
