The galaxy presents an elliptical morphology, appearing largely smooth in structure with a high degree of central concentration. A notable lack of distinct spiral arms or prominent dust lanes suggests it is likely an early-type galaxy. The color gradient shows a slightly more yellow/orange hue towards the galactic nucleus, likely indicating an older stellar population is more concentrated in the center. The outer regions appear slightly bluer, which may indicate the presence of a younger, though subdued, stellar population. Overall, the galaxy is reasonably luminous, suggestive of a fairly massive system with ongoing, albeit potentially low-level, star formation. There might be some minor irregularities present, hinting at a possible past interaction or disturbance, however, there is no evidence of a significant ongoing merger.
