The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its core is a bright, concentrated yellowish-white hue, with the light intensity gradually decreasing towards the outer edges. There is very little discernible structure, such as spiral arms or dust lanes, indicating a relatively well-mixed stellar population. The overall shape is generally round, with a slight elongation. The galaxy shows no obvious signs of recent or ongoing major mergers or tidal disturbances. Its color suggests a population of older stars, although some level of ongoing star formation activity cannot be ruled out.
