The galaxy presents a largely smooth, elliptical morphology. It appears as a centrally concentrated spheroid of light. There is some slight indication of asymmetry and a faint, diffuse halo extending outwards from the main body of the galaxy. The galaxy exhibits a somewhat irregular shape overall. The core is bright, suggesting a relatively high density of stars in the central region. There is a color gradient noticeable, transitioning from a more bluish hue in certain areas to a slightly redder color in the outer regions, potentially indicating varying stellar populations. The object is relatively isolated, with no immediately obvious signs of major interaction or merging activity, though some minor disturbance may be present.
