The galaxy presents as a slightly elongated, disk-like structure viewed at an oblique angle. Its central region is a bright, concentrated bulge, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy display a more diffuse, bluish-white color, indicating the presence of younger, hotter stars. The overall smoothness of the light distribution suggests a relatively evolved system, likely an early-type spiral or lenticular galaxy. There is a subtle indication of faint, loosely defined spiral arm structure within the bluer disk, though this is not sharply defined. The galaxy does not exhibit any obvious signs of recent major mergers or tidal disturbances, appearing relatively undisturbed.
