The galaxy presents a largely smooth, elliptical morphology. Its core is a bright, concentrated region of light, suggesting a high density of stars in the galactic center. The overall color profile is dominated by yellow and red hues, indicating an older stellar population with less active star formation. A faint tail or tidal feature extends from the main body of the galaxy, hinting at a possible past interaction or merger event. This feature exhibits bluer colors, which suggests the presence of younger stars that were either formed in situ as a result of the interaction, or stripped from another galaxy. The shape appears very round, with little elongation or distortion, though the faint tail disrupts the perfect symmetry.
