The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile with a gradual decline in brightness towards its outer regions, but appears to lack distinct features such as spiral arms or a prominent disk. The galaxy's shape is predominantly rounded, with only a slight deviation towards an elongated form. The galaxy core appears to be a singular body, with no distinct structures nearby indicating that it is in the process of merging with another galaxy. The color profile displays a central region of redder hue surrounded by a bluer ring; a possible indication of the central region containing older stars, while the surrounding regions may have pockets of more recent star formation.
