The galaxy presents as a relatively smooth, disk-like structure with a moderate inclination relative to our line of sight. It appears elongated, though not extremely so. The central region is somewhat brighter than the outer regions, suggesting a moderate concentration of stars towards the galactic nucleus. The color appears primarily bluish-white, which may indicate a population of relatively young, hot stars and ongoing star formation within the galaxy. There is no obvious spiral structure or bar visible in the image; it appears to be a relatively undisturbed system, with no obvious signs of major mergers or interactions.
