The galaxy presents as a generally smooth, elliptical-like structure. The central bulge is prominent and appears yellowish-white, indicating a population of older stars. The galaxy exhibits an overall high degree of smoothness, with no apparent spiral arms or dust lanes visible. It appears mostly round, although there is some slight elongation to the side. No major disturbances or signs of ongoing merger activity are readily apparent within the galaxy's morphology, although there is a small feature nearby, that could possibly indicate a past interaction. The galaxy has a substantial mass, which suggests that the star formation has been reduced in recent times. Overall, the galaxy appears to be a mature, relatively quiescent system.
