The galaxy appears as a smooth, elliptical-like object with a bright central bulge. There is a noticeable decrease in luminosity from the core outwards, suggesting a centrally concentrated mass distribution. The overall color is generally blue-white, hinting at a moderate presence of younger, hotter stars, or perhaps a blend of stellar populations. There is a slight elongation visible, implying a deviation from a perfectly spherical shape. No distinct spiral arm structures are visible, and the overall morphology suggests a relatively evolved galaxy. The lack of pronounced irregularities or tidal features suggests that it is likely undisturbed by recent major mergers, though some minor disturbance cannot be ruled out.
