The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. There is no immediately apparent spiral structure or disk. The galaxy exhibits a color gradient, transitioning from a yellow-white core to a slightly redder halo. The overall shape is moderately elongated, appearing somewhat oblate. There may be faint evidence of a minor disturbance, but no clear indication of an ongoing major merger. The galaxy's integrated light is dominated by older stellar populations suggesting a low rate of star formation.
