The galaxy presents as a smooth, centrally concentrated object. Its light profile suggests an elliptical morphology, lacking any discernible spiral arm structure or a prominent disk. The galaxy exhibits a radial color gradient, with a bright, yellowish core that fades to a redder hue in the outer regions. The isophotes appear largely elliptical, though some slight irregularities are visible. The relative homogeneity in color distribution indicates a potentially evolved stellar population. Faint, diffuse light extends outwards, suggesting the presence of a sparse halo. There is no indication of any ongoing major merger events or significant tidal disturbances.
