The galaxy presents as an elongated, disk-shaped structure viewed nearly edge-on. The central region exhibits a brighter, more concentrated luminosity profile indicative of a prominent bulge. The bulge appears rounded and smoothly transitions into the fainter, extended disk. There is a relative deficiency of resolvable star-forming regions throughout the galaxy. The color of the galaxy appears predominantly yellowish-orange. There is no obvious evidence of strong tidal interactions or major mergers in this image, however, there is evidence that minor disturbances may be present. The disk appears relatively uniform and thin, lacking distinct spiral arm structures or significant dust lanes. The galaxy appears relatively isolated in this field.