This galaxy presents as a flattened, disk-shaped system, viewed at an oblique angle. There is a central bulge, appearing as a concentration of light, with a yellowish white hue. The disk component exhibits a bluer tint, suggesting the presence of younger stars. A prominent dust lane is not readily apparent in this image; the galaxy appears to be fairly smooth. The galaxy appears elliptical, with an approximate ratio of its minor to major axis of roughly 0.4. Some slight disturbances can be seen in the outer edges of the disk. These are small and hard to characterize. The galaxy appears to be relatively isolated, with no obvious signs of interaction or major disturbance with other galaxies. The overall morphology leans towards a late-type spiral galaxy, with a relatively small bulge and loosely wound spiral arms that may be challenging to distinguish at the current resolution.