The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology. Its overall shape is elongated, but not highly cigar-shaped, with a somewhat rounded appearance. The light distribution is relatively uniform, lacking distinct spiral arms or prominent dust lanes. The galaxy's color gradient transitions from a yellowish-orange hue in the central region to a slightly bluer color in the outer edges. There is no evident sign of a recent or ongoing major merger event, though a subtle asymmetry or minor disturbance might be present in the outer halo. The overall impression is that of a mature galaxy with a dominant old stellar population, potentially possessing ongoing but subdued star formation.
