This galaxy appears to be a relatively smooth, elliptical system. It exhibits a bright, concentrated central bulge that gradually fades into a more diffuse halo. The core region appears yellowish, suggestive of an older stellar population. There is a faint, subtle bluer cast in the outer regions, which could indicate a small amount of recent star formation, or a difference in the stellar population between the inner and outer regions of the galaxy. The overall shape is mostly round. No strong tidal features or signs of ongoing major merger activity are readily apparent. There's a slight hint of possible minor disturbance in the symmetry, potentially indicating a past or minor merger event.
