The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The galaxy appears slightly elongated, displaying a shape somewhere between round and cigar-shaped. There is little evidence of spiral arms or significant disk features. The overall structure suggests a system that has undergone significant dynamical relaxation. There are no obvious signs of major mergers or tidal disturbances, though subtle features might be below the resolution limit. Hints of bluer regions can be seen around the edge of the core, showing hints of ongoing star formation in the galaxy.
