The galaxy presents as a centrally concentrated object, displaying a smooth, largely featureless morphology. The light distribution is generally elliptical, appearing moderately rounded with a slight elongation. A dominant, bright core is visible, suggesting a concentration of older stellar populations. Hints of a faint, diffuse halo are present surrounding the core region, which extends outwards. Faint disturbances are apparent, indicating possible interaction with smaller galaxies or a recent minor merger event. Overall, the galaxy appears to be relatively evolved, consistent with an early-type, elliptical galaxy.
