The galaxy appears to be a relatively smooth, elliptical system. Its overall shape is somewhat elongated. The galaxy exhibits a bright central bulge, which appears to be the brightest region. The luminosity decreases gradually from the center outwards, with no distinct spiral arm structures visible. The color is generally bluish-white, particularly in the inner regions, suggesting a moderate population of younger, hotter stars. The outer regions appear fainter and slightly redder. No obvious signs of major mergers or tidal disturbances are readily apparent, although there is a subtle asymmetry to its shape, possibly indicating a past interaction or minor disturbance.
