The galaxy presents as a flattened, elongated structure with a high degree of smoothness. The light distribution suggests a dominant central bulge surrounded by a fainter, more diffuse disk. The color gradient within the galaxy indicates a possible variation in stellar populations, with the central regions appearing slightly redder and the outer regions showing hints of bluer hues, possibly suggesting ongoing star formation. The galaxy exhibits a relatively undisturbed morphology, with no obvious signs of major mergers or significant tidal interactions. Overall, the galaxy appears to be an evolved system with a significant spheroidal component and a relatively quiescent star formation history.
