The galaxy presents as a roughly elliptical, disk-shaped structure with a bright, concentrated central bulge. There is an apparent disk component, displaying variations in color and luminosity indicative of differing stellar populations and gas distributions. The central region exhibits a notable concentration of intense blue-white light, suggesting the presence of active star formation or an Active Galactic Nucleus. The outer regions of the disk show a gradual decrease in surface brightness. Faint disturbances can be seen along the outskirts of the disk, appearing as subtle asymmetry. No prominent spiral arm structures are directly apparent in the image. The overall color profile suggests a composite stellar population with both older, redder stars and younger, bluer stars contributing to the observed light.
