The galaxy presents as a primarily smooth, elliptical-like structure. There is a concentration of light in the center, which fades gradually towards the outer regions. The galaxy exhibits a yellowish-orange hue, indicating a population of older stars. While the main structure is smooth, subtle irregularities are observed in the outer edges, hinting at possible minor disturbances or interactions. Overall, the galaxy does not appear to be experiencing a major merger event, but some low level disturbances are not excluded.
