The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. The color gradient suggests a population of older stars, with the core exhibiting a yellowish-orange hue, potentially indicative of a diminished rate of star formation. The isophotes display a nearly circular morphology, deviating minimally from a perfect sphere. There is little evidence of distinct spiral arms or significant dust lanes. Minor disturbances are potentially present. The overall appearance suggests a mature system with a substantial stellar mass.
