This galaxy presents a primarily smooth morphology. It appears elliptical in shape, with a noticeable, but subtle, elongation. The central region exhibits a high degree of concentration, appearing bright and possibly indicative of an older stellar population, which tends to be more yellow in color. There's little evidence of significant dust lanes or spiral arm structures within the visible light spectrum. No major disturbances or mergers are apparent in this image, though a slight asymmetry cannot be ruled out entirely. The galaxy's outskirts are relatively diffuse, fading gradually into the background sky. It exhibits a consistent color gradient from the core to the outer regions, implying a fairly well-mixed stellar population distribution.