The galaxy presents as a centrally concentrated object with a smooth morphology. The central region exhibits a bright, slightly off-white hue, suggesting a significant population of older stars. The overall shape appears largely circular, transitioning to a less defined, fainter halo region. There may be a hint of a faint disk structure present on the outer edges of the galaxy, though it lacks distinct features. There is no evidence of strong tidal interactions or merger activity, although a slight asymmetry could indicate some minor disturbance. The color gradient shifts gradually from the brighter central region to a redder outer halo, indicative of varying stellar populations. 
