The galaxy appears to be a relatively smooth, elliptical-like structure. The core region is a bright, yellowish-white, suggesting an older stellar population dominating the center, with little active star formation. The galaxy seems to transition from a yellow core to more reddish outskirts, implying some spatial variation in stellar populations or dust content. The galaxy's shape appears moderately elliptical rather than perfectly spherical. There is little to no indication of spiral arms or a significant disk component. There is no obvious evidence of any ongoing major mergers or significant tidal disturbances affecting the galaxy's overall form.
