The galaxy presents as a largely featureless elliptical or spheroidal system, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-orange hue, suggesting an older stellar population and relatively low levels of ongoing star formation. A diffuse greenish glow extends outwards from the central region, potentially indicating the presence of ionized gas or a younger population of stars compared to the core. The galaxy appears relatively isolated, showing no significant tidal features or morphological disturbances indicative of recent major merger activity. Its overall shape appears quite round with a slight elongation.
