The galaxy presents as a single, largely featureless entity. It exhibits a centrally concentrated morphology with a high degree of symmetry, appearing almost perfectly circular in projection. The core is bright, suggestive of a high stellar density or possible AGN activity. The color gradient transitions gradually from a bluer-white core to a reddish-orange outer halo. There is no apparent spiral structure, bar, or dust lane. The overall smooth appearance and radial color gradient indicate an evolved system, potentially an elliptical galaxy with ongoing, but likely low, star formation. No signs of tidal disturbances or major mergers are visible, although a very slight asymmetry in the outer halo cannot be entirely ruled out. The galaxy appears relatively isolated.
