The galaxy presents an edge-on disk morphology. A prominent dust lane bisects the galaxy's light, obscuring the central bulge. The bulge appears elongated and slightly boxy. The overall color suggests an older stellar population, with a yellowish hue dominating the visible light. Faint, blueish star formation is visible on one side of the disk, suggesting ongoing, though limited, star formation. There are no obvious signs of a major ongoing merger or significant tidal disturbances. The galaxy appears relatively isolated.
