The galaxy appears to be a spiral galaxy, viewed at an oblique angle. It exhibits a noticeable bulge at its center, displaying a smooth, concentrated distribution of light. The arms are not sharply defined, and appear somewhat flocculent and tightly wound, contributing to a disk-like appearance. Color gradients are subtly present, with a yellowish hue towards the central bulge, suggesting an older stellar population, and a bluer tint in the outer regions, indicative of more recent star formation. There's no apparent sign of an active galactic nucleus, and no major disturbances or merging events are visible. It appears as a relatively isolated galaxy.
