This galaxy presents as a spiral galaxy with a prominent central bulge. The bulge appears relatively smooth and exhibits a yellowish-white hue, suggesting an older stellar population. The galaxy shows a disk-like structure surrounding the bulge, and a degree of organized structure which indicates the presence of spiral arms, but these arms are not sharply defined, appearing somewhat flocculent. The disk is slightly inclined with respect to our line of sight. There are no major disturbances noted, although some possible minor interaction is not excluded. Overall, the color gradients suggest a decreasing age of stellar population from the bulge towards the outer disk.
