The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high surface brightness, appearing yellowish-white in color, suggesting a concentration of older stars and potentially a supermassive black hole. Moving outwards from the core, the color gradually shifts towards a redder hue, indicative of an aging stellar population. There are only subtle features, with no apparent spiral arms or distinct dust lanes visible in this image. The overall shape is close to round, but slightly elongated. There is no indication of any significant ongoing merger activity or major disturbances in the galaxy's structure.
