The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, centrally concentrated light profile. The overall color is yellowish-white, indicative of an older stellar population dominating the light emission, although some bluer regions are present. The shape is not perfectly spherical, showing a slightly elongated, flattened appearance. No prominent spiral arm structures or dust lanes are discernible. There is no obvious evidence of a strong ongoing merger, although subtle asymmetries might suggest a previous minor interaction or disturbance. The galaxy is relatively compact, appearing concentrated in the image.
