The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy given the lack of discernible spiral arms. It exhibits a bright, yellowish core, which suggests an older stellar population dominates the central region. The color gradient transitions to a slightly bluer hue in the outer regions, indicating the potential presence of younger stars or ongoing, albeit limited, star formation. The overall morphology is generally undisturbed with a possible minor gravitational interaction with a faint region of light to the right of the galaxy. Given the color profile and lack of strong dust lanes, the galaxy seems to be in the process of passively evolving.
