The galaxy presents as a faint, elongated lenticular or possibly spiral structure viewed at an oblique angle. The central bulge appears moderately bright and concentrated, with a seemingly smooth distribution of light. Extending outward from the bulge, a faint, disklike component is visible. There is a hint of possible spiral arm structure, however it's not well defined, indicating a likely flocculent or possibly disturbed spiral galaxy or smooth disk galaxy with no spiral arms. The overall color is bluish. There is no evidence of a prominent dust lane or significant star formation regions. The galaxy appears relatively undisturbed, however there is some low probability it is a minor merger, and appears likely to be nearing the end of star formation. The galaxy does not have a sharp boundary but rather fades gradually into the background.
