The galaxy presents as a centrally concentrated object with a smooth overall appearance. Its morphology appears to be largely elliptical, though some asymmetry is present. A subtle elongation is noticeable, deviating slightly from a perfectly circular shape. The light distribution is centrally peaked, with a gradual decrease in brightness moving outward from the core. The galaxy displays an overall bluish-white hue near the core which fades to a more red color on the outer edges, suggestive of differing stellar populations and age gradients. There appears to be some subtle evidence of a disk-like structure embedded within the main body, but this is not obvious. There is no obvious spiral arm structure nor prominent dust lanes visible in this image. The galaxy seems undisturbed, showing no signs of major recent mergers or tidal interactions.
