The galaxy presents as a primarily smooth, elliptical structure. The core exhibits a high degree of luminosity, appearing a bright yellow-white, indicative of a dense population of older stars. The galaxy's luminosity decreases gradually moving outwards from the core, transitioning to a more diffuse, slightly bluer halo. There are some subtle hints of disk like components within the structure, though this is not necessarily a spiral galaxy. There is a very slight disturbance to its overall form and a hint of what could be considered a minor tidal feature.

Based on the color profile, the galaxy appears to have ongoing, low levels of star formation, with a population of younger stars contributing to the blue wavelengths in the outer regions. 
