The galaxy presents as a largely featureless, elliptical structure with a high degree of central concentration. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. Moving outward from the core, the galaxy displays a smooth, gradual decline in surface brightness. There is minimal evidence of spiral arms or significant dust lanes, but a subtle bluing of the outer regions indicates the presence of some younger, hotter stars. The overall morphology suggests a system that is relatively relaxed, without any significant signs of recent major mergers or tidal disturbances. The rounded appearance dominates, with only a subtle deviation from perfect circularity. The galaxy exhibits a redshift indicating that it is relatively close to us. 
