The galaxy presents as a somewhat flocculent spiral galaxy, with hints of spiral arms, though not sharply defined. The central bulge appears prominent and yellowish-white, indicating an older stellar population. Moving outward, the disk shows a bluer tint, suggesting ongoing star formation. There's a slight asymmetry to the disk, which could suggest a minor interaction with another galaxy or an internal disturbance. Overall, the galaxy has a relatively high mass and star formation rate.
