The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. Its overall shape is moderately elliptical, not perfectly spherical, with an approximate axis ratio of perhaps 3:2. The color gradient suggests a population of older stars, exhibiting a yellowish to reddish hue, concentrated towards the galactic center. There is no visible spiral arm structure or dust lane obscuration. There appears to be a gradual decrease in luminosity from the center outwards, indicating a centrally concentrated stellar distribution. There is no evidence of any major ongoing merging events or tidal disturbances, suggesting the galaxy is relatively undisturbed. The galaxy presents a fuzzy edge rather than a sharp one, indicating a presence of a large halo.
