The galaxy presents as a centrally concentrated, relatively smooth, and featureless object. The morphology is generally elliptical or spheroidal, displaying a high degree of roundness. There is minimal evidence of a disk structure or spiral arms. The light profile appears to diminish smoothly from the bright central core outwards. There is no indication of ongoing major mergers, although some minor asymmetry or disturbance cannot be completely ruled out. Color gradients appear subtle, with the central region exhibiting a somewhat yellower or redder hue, and the outer regions appear slightly bluer. The overall structure suggests a relatively evolved system with a low rate of star formation.
