The galaxy presents a morphology dominated by a smooth, centrally concentrated structure. It displays a yellowish-orange hue in the central region, suggesting an older stellar population and minimal ongoing star formation in the nucleus. Fainter, slightly bluer regions are subtly present, hinting at possible, low-level star formation within localized areas. The overall shape is somewhat elliptical, though with subtle irregularities suggesting potential gravitational interactions or internal disturbances. There is a possible merging event or minor disturbance. The main body is somewhat more round. There are no well defined spiral arms.
