The galaxy presents as a relatively smooth object, elliptical in appearance. A bright, concentrated central bulge dominates the structure, fading outwards into a less defined, more diffuse halo. There are no obvious spiral arms or prominent dust lanes visible. The color is predominantly bluish-white, which may suggest a population of younger, hotter stars, or an active galactic nucleus. However, the smooth morphology is not indicative of recent major merger activity, though minor disturbances cannot be ruled out based on the image alone. The overall appearance leans toward an early-type galaxy.
