The object presents as a relatively smooth, elliptical-shaped galaxy, exhibiting a high degree of central concentration. The core region is notably luminous, displaying a bright yellowish-white hue. The light gradually diminishes in intensity moving outwards from the center, transitioning to a more diffuse and reddish-orange color in the outer regions. No distinct spiral arm structures or dust lanes are discernible. The overall appearance suggests a mature galaxy dominated by an older stellar population with little to no ongoing major merger activity. There are potentially very faint, subtle disturbances in the outer halo but further investigation is necessary to confirm the nature of these features.
