The galaxy presents an elliptical morphology, appearing more elongated than perfectly spherical. It displays a smooth, concentrated light profile, with a bright, yellowish core that gradually diffuses outwards. The outer regions of the galaxy exhibit a fainter, more indistinct glow. No distinct spiral arm structures or dust lanes are discernible. There appears to be a minor gravitational disturbance, with a slight asymmetry observed in the outer halo. The galaxy likely has a considerable stellar mass, but shows only a low rate of star formation.
