The galaxy presents as a largely elliptical form, demonstrating a high degree of central concentration. Its overall morphology appears smooth, lacking prominent spiral arms or significant dust lanes. The light distribution gradually decreases from a bright, concentrated core outwards to the galaxy's diffuse edges. The color is generally yellowish, indicative of an older stellar population. There is no strong evidence of recent major merger activity or tidal features. Minor perturbations cannot be ruled out given the image quality.
