The galaxy appears to be a relatively smooth, elliptical structure, exhibiting a centrally concentrated luminosity profile. The core region is bright and gradually fades into a diffuse halo. Its overall shape is generally round, showing minimal signs of elongation or distortion. There are no clearly discernible spiral arms or prominent dust lanes visible in this image. Some subtle color variations are observed, with a slightly bluer tint in the outer regions compared to the more yellow-white core, possibly indicating differing stellar populations. The galaxy shows hints of disturbance, but no strong signs of an ongoing or recent major merger event. The lack of strong star formation regions is consistent with an older stellar population dominating its overall light.
