The galaxy presents as a centrally concentrated, elliptical system. The core exhibits a high surface brightness and a yellowish hue, suggesting a population of older stars. The overall morphology is smooth and rounded with a lack of readily discernible spiral arm structures or dust lanes. The outer regions of the galaxy show a gradual decrease in luminosity, fading into the background sky. There is no indication of any major ongoing mergers or significant tidal disturbances. Subtle color variations within the galaxy suggest differing stellar populations and/or metallicities between the core and halo regions. 
