The galaxy presents a largely smooth, elliptical morphology. It appears somewhat round in shape, with a radial intensity profile that increases toward the center, lacking any prominent disk structure or spiral arms. There are hints of very minor disturbance around the central region. The galaxy exhibits a color gradient, transitioning from a redder core to slightly bluer outer regions. The galaxy is fairly isolated, showing no signs of ongoing major merger activity or significant tidal interactions with nearby companions. The lack of readily discernible features and the smooth light distribution suggest a relatively evolved stellar population and a low star formation rate.
