The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance. The light profile suggests an elliptical morphology. The galaxy's core is notably bright and appears yellowish-white. The outer regions of the galaxy exhibit a redder hue, indicating a potential population of older stars or a higher dust concentration. The overall structure appears undisturbed, with no obvious tidal features or signs of ongoing mergers. The object does not present any significant disk-like features, and the light distribution is relatively symmetrical.
