The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a high surface brightness concentration, with luminosity decreasing towards the outer edges. The galaxy appears somewhat elongated, deviating slightly from a perfect circular shape. Color gradients are subtle, with a suggestion of redder hues concentrated in the core and a slight shift towards bluer tones in the extended halo. There is no visually apparent evidence of recent or ongoing major mergers or significant tidal disturbances, although subtle irregularities could indicate minor interactions. Overall, it appears as a mature system with little ongoing star formation.
