The galaxy appears as a centrally concentrated object with a relatively smooth, round morphology. There is no strong indication of a distinct disk structure or spiral arms. The light distribution suggests an elliptical or lenticular type galaxy. The central region of the galaxy exhibits a bright, yellowish-white glow, indicating a concentration of older stellar populations, or potentially a low level active galactic nucleus. Faint color gradients are present, with a slightly bluer hue around the central region. The overall shape shows no obvious signs of major mergers, however there is a suggestion of minor disturbances. These features suggest a galaxy that may have experienced some past interaction or minor merger events that are still visible through asymmetries in the light distribution. The galaxy shows evidence of recent or ongoing star formation.
