The galaxy appears as an edge-on spiral, characterized by a prominent, thin disk. The disk displays a relatively smooth texture with slight obscuration possibly due to dust lanes, suggesting ongoing star formation. The central bulge is visible, appearing somewhat elongated and exhibits a color profile that leans towards redder wavelengths, indicating an older stellar population. The overall color of the galaxy is generally consistent, with the central bulge appearing more concentrated in older stars than the disk. There is no visible active galactic nucleus or signs of recent major merger events. Minor asymmetries within the disk structure may suggest minor gravitational interactions or disturbances. The structure seems relatively undisturbed otherwise.
