The galaxy appears to be a relatively compact object. The light profile suggests a centrally concentrated morphology, potentially indicative of an elliptical or lenticular galaxy. There is a bright, yellowish core that fades into a slightly bluer, less distinct halo. No clear spiral arm structure or prominent dust lanes are discernible within this image, reinforcing the possibility of an early-type galaxy classification. There might be a subtle, low-surface-brightness disk, though the overall impression is of a system dominated by a smooth, spheroidal component. The colors suggest a relatively old stellar population with ongoing, but not exceptionally high, star formation. There is no obvious indication of a major merger event. Minor disturbances cannot be ruled out, but the overall appearance is fairly quiescent.
