The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its color is predominantly yellowish-white, suggestive of an older stellar population. There are no discernible spiral arms or significant dust lanes. The light profile appears relatively uniform, lacking distinct substructures within the galaxy body. There is no evidence of a recent or ongoing major merger event, though there is potentially a minor irregularity in the distribution of light to the lower left. The overall impression is that of a relaxed system, likely a galaxy that has undergone significant evolution. The estimated effective radius suggests it is of moderate size, but the luminosity implies it is relatively bright for its size.
