The galaxy appears to be an elliptical galaxy. It exhibits a smooth, centrally concentrated morphology with a bright core that quickly fades into the outer regions. The shape is largely spherical, with minimal deviation from perfect circularity, although there is a subtle elongation. No distinct spiral arms, dust lanes, or other features indicative of active star formation or a disk component are discernible. The galaxy's color profile suggests a population of older stars, as evidenced by the yellowish hue. There is no sign of recent mergers or major tidal disturbances.
