The galaxy presents an elliptical morphology, with a relatively smooth appearance across its extent. The core region exhibits a brighter luminosity, suggesting a higher density of stars and interstellar material. The light distribution appears primarily concentrated towards the center, with a gradual decrease in intensity towards the outer edges. There is a slight suggestion of tidal disruption in the immediate vicinity of the galaxy, possibly indicating an ongoing or recent interaction with another galaxy. This interaction is potentially characterized by faint trails or distortions in the galaxy's outer halo. Overall, the galaxy shows evidence of a relatively evolved system that has likely experienced some environmental influence. 
