The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated. The light distribution suggests a fairly well-defined spheroidal structure, with the isophotes becoming gradually more elliptical as the radius increases. The central region exhibits a yellowish-orange hue, indicative of an older stellar population. Progressing outwards from the core, the galaxy transitions towards bluer colors, although the overall color gradient is subtle. There is no readily apparent spiral arm structure or dust lane obscuration within the galaxy. No signs of tidal tails or strong distortions are visible in the image.