The galaxy appears as a diffuse, elliptical object. The central region exhibits a brighter, concentrated luminosity, suggestive of a galactic bulge. The outer regions display a gradual decrease in brightness, indicating a fading stellar population or lower density of luminous matter.

There is a faint, elongated structure extending from the main body of the galaxy, possibly a tidal tail or a disrupted arm. The galaxy's overall color is predominantly neutral. Patches of subtle color variation may indicate areas of differing stellar populations or dust obscuration.

The morphology suggests a relatively undisturbed system, although subtle features might point towards minor past interactions or internal dynamical processes. Further analysis is needed to determine the exact nature of the fainter structural elements and the galaxy's evolutionary history.
