The galaxy presents as a centrally concentrated object with a diffuse halo. The central region exhibits a slightly elliptical morphology, appearing largely smooth in texture. There is a hint of a faint disk-like structure, or at least a deviation from perfect sphericity, along its major axis. The galaxy's color profile suggests a population of intermediate to older stars dominating the light output. The galaxy overall is a blueish-white, with faint hints of redder regions, possibly indicative of areas with ongoing star formation. The overall light distribution is very smooth, implying little dust obscuration. The galaxy does not show any obvious signs of major interactions or tidal disturbances, though there is a suggestion of minor asymmetry, potentially from a smaller past interaction. There is a slight elongation that suggests a merging history, but it is not heavily distorted.
