The galaxy presents an elliptical morphology, exhibiting a smooth and relatively featureless structure. The central bulge appears prominent and concentrated, with a luminous golden hue that gradually fades into the surrounding disk. The light distribution suggests a high degree of symmetry, lacking any obvious spiral arms or bar-like structures. No major disturbances or tidal tails are visible, although there may be some minor irregularities in the outer regions. The overall color indicates a population of older stars, with a low rate of ongoing star formation. The galaxy displays a compact size, with a well-defined edge and a smooth transition into the background sky.
