The galaxy presents a disk-like structure with a prominent central bulge. The galaxy is viewed at an oblique angle, exhibiting a tilt relative to our line of sight. Spiral arm structures are present, though somewhat tightly wound. Dust lanes are subtly visible within the disk, contributing to its mottled appearance. The central bulge appears bright and yellowish-white, indicating a population of older stars. The disk displays a bluer hue, suggesting the presence of younger stellar populations and ongoing star formation. Overall the galaxy has a smooth, ordered appearance with a bright, centralized light profile. The galaxy is approximately 6.1 kpc in radius.
