The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution. The core region exhibits a concentrated luminosity, appearing yellowish, suggesting an older stellar population and reduced current star formation. The outer regions of the galaxy appear more greenish in hue. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major merging events. The shape is not perfectly circular, but rather slightly elongated, indicating a possible deviation from perfect isotropy.
