The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. There is a subtle color gradient extending outwards from the core, transitioning to a slightly redder, less luminous halo. No distinct spiral arms or prominent dust lanes are apparent. The overall shape is nearly circular. There are no clear signs of ongoing major merger activity or significant tidal disturbances in its immediate vicinity. Faint extensions or low surface brightness features may exist.
