The galaxy presents as a relatively smooth, elliptical-like object. Its overall color appears slightly reddish, suggesting an older stellar population with fewer hot, young stars. The light distribution appears fairly uniform, with a gradual decrease in intensity from the center outwards. There is a subtle hint of a possible disk, but the dominant impression is of a spheroidal structure. No prominent spiral arms or distinct star-forming regions are discernible. There is a faint suggestion of a tidal tail or minor disturbance to the structure, but this could be the effect of noise. The galaxy appears isolated, without obvious signs of recent or ongoing merging activity. The overall morphology indicates a galaxy that has likely undergone significant evolution and quiescence.
