The galaxy presents as a generally smooth, elliptical-like morphology. The central region exhibits a high concentration of light, appearing bright yellow-white in color and gradually diffusing into the surrounding area. There is a slight elongation, suggesting it is not perfectly spherical. The outer regions appear to be less luminous, with a mottled, blueish color, hinting at possible faint, younger stellar populations. There is no evidence of spiral arm structure or significant dust lanes are observed. Minor disturbances are possibly present, but no major distortions are visible, and the galaxy appears to be largely isolated.
