The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The overall shape is approximately elliptical, though it exhibits a slight departure from perfect sphericity, appearing somewhat in between round and cigar-shaped. There is little evidence of spiral arms or a distinct disk structure. Faint color gradients are visible, with the central region appearing more yellowish-white, suggesting an older stellar population. The outer regions show hints of blue, possibly indicating some ongoing, albeit low, level of star formation activity. No major signs of tidal disturbances or ongoing merger events are discernible, suggesting the galaxy is relatively undisturbed.
