The galaxy presents as a slightly elongated, disk-like structure, viewed at an oblique angle. It appears largely smooth in texture, suggesting a well-evolved system. A central bulge region is evident, exhibiting a more concentrated, yellow-white hue. The outer regions show a more diffuse and bluer tint, potentially indicating the presence of a younger stellar population or ongoing star formation. There may be a slight warp or asymmetry in the disk. There is no obvious signs of active galactic nuclei (AGN) activity or major disturbances within the image, although minor disturbances are possible.
