The galaxy appears to be a luminous elliptical, with a smooth, featureless morphology. Its overall shape is generally round with no obvious signs of a disk structure. The color gradient indicates a relatively old stellar population, with a yellowish core suggesting a concentration of evolved stars. There is no obvious dust lane or spiral arm structure evident in the image. There are no tidal tails or distorted features to suggest a recent major merger event, although it does have some faint disturbances, possibly caused by a minor merger event. It exhibits a significant luminosity, indicative of a massive galaxy with a high stellar mass and relatively low star formation rate.
