This galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is elliptical, though slightly elongated. The core of the galaxy exhibits a bright, yellowish-white color, suggesting a population of older stars. Moving outward from the core, the color transitions to a bluer hue, possibly indicating some ongoing, albeit moderate, star formation within a disk-like component. The absence of clear spiral arms, distinct dust lanes, or irregular structures supports the classification of this galaxy as primarily elliptical, with the possibility of a weak disk component. There is no strong evidence of any recent major merger activity, but a minor interaction or disturbance can't be ruled out. Overall, the galaxy seems to be a mature system with low star formation.
