The galaxy presents as a somewhat elongated spheroid with a generally smooth appearance. The central region exhibits a concentrated luminosity, appearing as a bright, yellowish core. A gradual decrease in brightness extends outwards from the center, with a subtle change in color to reddish hues at the outer edges. There is no discernible spiral structure or prominent dust lanes visible. The galaxy appears to be relatively isolated with no obvious signs of ongoing major mergers, although minor disturbances cannot be ruled out. The overall morphology suggests an elliptical or lenticular galaxy type at an approximate distance, as suggested by the measured redshift. It shows signs of low star formation rate.
