The galaxy presents as a centrally concentrated, elliptical morphology. It appears relatively smooth in texture, lacking prominent spiral arm structures or significant dust lanes. The light profile suggests a concentrated bulge component. There is a subtle color gradient, with the central region exhibiting a yellowish-orange hue, potentially indicating an older stellar population, while the outer regions display a slightly bluer tint. The overall ellipticity is moderate, showing a deviation from a perfect circular shape. There is no visible evidence of a major ongoing merger event, although subtle asymmetries in the outer halo cannot be entirely ruled out.
