The galaxy presents a smooth, elliptical morphology. It appears centrally concentrated with a bright, yellowish core that gradually fades into a diffuse halo. The galaxy exhibits an elongated shape, appearing more "in between" than perfectly round. There is no apparent spiral structure or distinct dust lanes visible in this image. The overall color gradient suggests an older stellar population. There are no obvious signs of a major merger event or strong tidal interactions. Minor disturbances cannot be ruled out at this resolution, though the overall impression is that of a relatively undisturbed, evolved system.
