The galaxy appears as a centrally concentrated elliptical, exhibiting a smooth, relatively featureless morphology. The core of the galaxy presents a bright, yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness, with the color transitioning towards a reddish-yellow. The overall shape is moderately round, with no discernible spiral arms or distinct features. There is no visible evidence of a major merger event or tidal disturbances affecting the galaxy's structure, although some minor asymmetrical features are observed on close inspection. These characteristics suggest a relatively evolved system, potentially a massive elliptical galaxy with a reduced rate of star formation.
