The galaxy presents as a centrally concentrated, elliptical morphology with a smooth, diffuse light distribution. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation within the nuclear region. The overall shape appears generally round, with a slight deviation towards an intermediate ellipticity. There's faint evidence of some minor structural disturbance or asymmetry on one side, which may indicate a past interaction. The outer regions display a gradual decrease in luminosity and appear slightly bluer compared to the core, perhaps hinting at a small population of younger stars in the galactic periphery. The galaxy's color indices indicate a redder overall spectral energy distribution.
