This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a bright, concentrated central bulge that fades into a more diffuse halo. The galaxy's overall shape is elongated. There appears to be a slight disk structure with some features present. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, potentially indicating a lower rate of star formation. There may be minor disturbances nearby but it does not show any sign of actively merging with another galaxy.
