The galaxy presents an overall elliptical morphology, appearing mostly smooth and relatively undisturbed. There is a central bright bulge exhibiting a yellow-white hue, indicating a concentration of older stellar populations. The outer regions of the galaxy are fainter and show a subtle shift towards bluer tones, possibly signifying some ongoing, though limited, star formation. No distinct spiral arm structures are visible. The shape is moderately elliptical, deviating slightly from a perfectly circular form. There's no obvious evidence of strong tidal interactions or recent major mergers, although some subtle distortions could suggest minor past disturbances. The galaxy appears relatively compact, with a well-defined edge beyond which its luminosity rapidly decreases.
