The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. A subtle, diffuse halo surrounds the core, with a gradual decrease in luminosity towards the outer edges. There is a slight elongation, hinting at an ellipsoidal rather than perfectly spherical shape. No distinct spiral arms or prominent dust lanes are discernible. The overall color profile suggests a relatively quiescent galaxy, likely with a low rate of star formation. No apparent signs of ongoing mergers or tidal disturbances are observed.
