The galaxy presents as a somewhat elliptical, smooth, and concentrated distribution of light. It is characterized by a distinct color gradient, exhibiting a yellowish-orange hue at its core, which transitions to a bluer tone in the outer regions. The morphology suggests an evolved stellar population concentrated centrally, with younger stars forming in the outer regions. The overall shape indicates a relatively undisturbed system, lacking prominent spiral arms or irregular features. No signs of active galactic nuclei activity are immediately apparent from the image. The galaxy appears as a relatively isolated object, showing no major signs of tidal interactions or ongoing mergers with nearby systems. The light distribution is relatively symmetrical, with a possible slight elongation, indicating a potential deviation from perfect circularity.
