The galaxy presents as a centrally concentrated elliptical type system. It exhibits a smooth, diffuse morphology with a high degree of circularity. The color profile suggests an older stellar population, dominating the central region. Fainter bluer hues surround the center, perhaps suggesting areas of younger stars or more recent star formation than the core. There appears to be a very slight tidal interaction or minor disturbance present. Otherwise the structure is generally undisturbed, presenting as a relatively mature system.
