The galaxy presents as an elongated, disk-shaped structure oriented nearly edge-on relative to our line of sight. A prominent central bulge is visible, appearing smooth and concentrated. The bulge dominates the light profile, particularly in the central region. The disk appears relatively thin and elongated, with a suggestion of some dust lane obscuration along the plane of the galaxy, although this is subtle. The disk fades in intensity further from the galactic center. The overall color is a relatively uniform yellowish-orange, suggesting an older stellar population throughout the galaxy. There is no obvious sign of recent star formation, such as bright blue regions or distinct spiral arm structure. The morphology suggests a likely classification as a spiral galaxy viewed edge-on. Further analysis using multi-band photometry and spectroscopy would be needed to confirm the morphological type and further characterize the stellar populations and dust content.
