The galaxy presents as an elliptical structure with a smooth, mostly featureless morphology. The core region appears bright and concentrated, suggesting a high density of stars. Progressing outwards from the core, there's a gradual decrease in luminosity, without any apparent spiral arm structures or dust lanes. The color profile is generally redder, implying a population of older stars and reduced current star formation activity. There is no obvious evidence of any major gravitational disturbances or ongoing merger activity, such as tidal tails or asymmetric features. The overall shape is more rounded than elongated.
