The galaxy appears as a somewhat elongated, disk-like structure with a noticeable central bulge. Its overall color is yellowish-orange, indicating a significant population of older stars and possibly a lower rate of current star formation. The galaxy displays some evidence of spiral arm structure, albeit somewhat faint and diffuse, rather than well-defined arms. These arms contribute to a disk that has a slight warp or asymmetry. There may be some dust lanes visible within the disk, further obscuring the spiral structure. The smoothness of the galaxy suggests an older stellar population, although a small amount of star formation is also possible. There might be a minor interaction or disturbance evident in the overall shape, but the primary morphology appears relatively undisturbed.
