This galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and centralized light distribution. The core is bright and yellowish in color, indicating a concentration of older stellar populations. The overall shape appears roughly circular, but with slight deviations from perfect symmetry. There are no visible spiral arms or prominent dust lanes. A very faint, diffuse halo surrounds the central region, gradually fading into the background sky. Subtle color variations suggest some variation in stellar populations or metallicity across the galaxy, although the limited resolution makes detailed analysis challenging. There is no strong evidence of a recent major merger, although some minor tidal disturbances cannot be ruled out based on this image alone.
