The galaxy presents as a somewhat symmetrical, though not perfectly circular, elliptical structure. The light distribution suggests a concentration towards the core, which is markedly brighter and more diffuse than the surrounding regions. There is evidence of some blue light in the outer portions of the galaxy, suggesting pockets of ongoing or recent star formation, though the overall color is more consistent with an older stellar population. Faint, elongated structures or tidal features are not obviously visible, but some asymmetry in the outer isophotes hints at possible past interactions.
