The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits a subtle color gradient, with a yellowish-white core transitioning to a bluer outer halo. There is a slight deviation from perfect circularity, hinting at a possible minor interaction or internal disturbance, though the overall structure remains largely undisturbed. The lack of distinct spiral arms or prominent dust lanes suggests a morphological classification toward the earlier end of the Hubble sequence. Its radial profile indicates a decline in surface brightness from the core outwards, typical of elliptical galaxies, with no prominent star-forming regions visible in the image. 
