The galaxy presents a smooth, elliptical morphology. Its color profile suggests the presence of a bulge consisting of older stellar populations, with bluer colors visible in the outer regions. The galaxy exhibits a moderate concentration of light towards the center, characteristic of an elliptical galaxy. There is little evidence of dust lanes or significant star formation activity within the galaxy, which implies that this is a mostly quiescent system. No apparent signs of recent or ongoing mergers are evident. The galaxy's shape appears somewhat elongated, but generally exhibits moderate rounding.
