The galaxy presents as a centrally concentrated, luminous object, exhibiting a smooth, elliptical morphology. It is generally round, though there is a slight elongation evident in its shape. The core region is considerably brighter and more concentrated than the surrounding outer regions. The galaxy's color profile suggests a population of older stars, contributing to its yellowish hue. There is little evidence of spiral arm structures, though subtle features hint at minor disturbances. No apparent signs of a major ongoing merger are readily visible. The light distribution is relatively uniform, transitioning smoothly from the core outwards, with no prominent dust lanes or distinct star-forming regions immediately obvious in this image.
