The galaxy presents as a relatively smooth, elliptical structure. It exhibits a prominent central bulge that appears yellow-white in color, suggesting a population of older stars. The light distribution smoothly decreases from the center outwards. The galaxy is elongated, with a major axis significantly longer than its minor axis, indicative of a prolate spheroid shape. No distinct spiral arms or significant dust lanes are apparent. There is no obvious evidence of recent major merger activity or significant tidal distortions in this image. Faint blue-ish hues are observed towards the outer edges, which may be indicative of younger stellar populations in those regions. The overall color suggests a galaxy that is relatively quiescent in terms of star formation.
