The galaxy presents as a spiral type, viewed at an oblique angle. It displays a prominent central bulge that appears relatively smooth and concentrated in light, indicating a higher density of older stellar populations. The disk component exhibits a bluer hue compared to the bulge, suggesting ongoing star formation. Faint spiral arm structures extend outwards from the central bulge, and are tightly wound. The galaxy lacks any obvious signs of major mergers or significant tidal disturbances. The disk appears somewhat flocculent, with varying degrees of light intensity.
