The galaxy presents as a largely homogenous, elliptical structure. It exhibits a high degree of central concentration, with the luminosity gradually decreasing from the core outwards. The galaxy appears relatively smooth, lacking significant, distinct features like spiral arms or prominent dust lanes. Its overall color is slightly yellow to green, which suggest a moderate population of older stars. There is little evidence of ongoing, intense star formation in this optical view. The isophotes are generally round. There are no obvious signs of tidal disturbances or interactions with other galaxies, such as extended plumes or distorted morphology. The galaxy appears to be a relatively isolated system.