The galaxy exhibits a lenticular morphology, appearing as a flattened disk-like structure viewed at an oblique angle. The central bulge appears relatively prominent and concentrated, displaying a yellowish hue, suggesting an older stellar population. The disk component is elongated and shows hints of a spiral structure, though it's not well-defined. There is a subtle blue tint on the edges of the disk, potentially indicative of some ongoing star formation. The galaxy does not show any signs of major mergers or significant tidal disturbances.
