The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light distribution. The central region displays a bright, yellowish core, which likely indicates a high concentration of older stars. The overall shape is somewhat elongated, deviating slightly from a perfect circular form. There are no prominent spiral arms or distinct features indicative of active star formation. A faint, diffuse halo surrounds the brighter central region. The lack of significant dust lanes or other irregularities suggests it is relatively undisturbed and not undergoing a major merger.
