The galaxy presents as a relatively smooth, disk-like structure with a slight inclination relative to our line of sight. Its overall color appears yellowish-white, suggesting a population of older stars. There is a distinct, brighter central region, perhaps indicative of a bulge or active galactic nucleus. A hint of bluer light exists at the edges of the disk which may represent younger star formation regions. The outer regions of the galaxy fade gradually into the background sky, indicating a lack of a sharp boundary to the galactic disk. The galaxy exhibits no obvious signs of major morphological disturbances or tidal interactions. The overall shape appears close to circular.
