The galaxy presents as an elongated, disk-shaped system viewed at a significant inclination. A bright, concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population. The galactic disk appears relatively smooth, with faint spiral arm structures that are difficult to resolve given the viewing angle. The outer regions of the disk show a bluer color, indicative of younger, hotter stars and potential ongoing star formation. Dust lanes are not clearly visible, but a subtle obscuration may exist along the disk. Overall, the galaxy appears to be a late-type spiral system, characterized by a moderate bulge and a thin disk exhibiting limited star formation.