The galaxy presents a generally smooth, rounded morphology. There is a slight central concentration of light, appearing as a subtle brightening towards the core. The overall color suggests a population of older stars, with some evidence of bluer regions that could indicate ongoing or recent star formation, or a population of hot, old stars. The galaxy's disk may not be apparent in the image, as it is an elliptical galaxy. There are no indications of strong tidal features or significant distortions that would suggest a major ongoing merger event, though some minor disturbances can be seen. This galaxy can be classified as a large elliptical galaxy.
