The galaxy appears to be a spiral galaxy viewed at an oblique angle, closer to edge-on than face-on. There's a prominent central bulge that exhibits a yellow-orange hue, potentially indicative of an older stellar population. Faint spiral arms emanate from the central bulge, appearing somewhat loosely wound. The arms are not sharply defined, appearing more diffuse and patchy. Dust lanes are likely present, contributing to the mottled appearance of the disk, but are not clearly discernible in the image. There is no obvious ongoing major merging activity or significant tidal disturbances present. The disk appears relatively undisturbed. Overall, it appears to be a fairly normal spiral galaxy.