The galaxy appears to be a relatively smooth, elliptical galaxy with a generally rounded shape. There are no obvious spiral arm structures or significant dust lanes visible in this image. The galaxy exhibits a moderate concentration of light towards its center. There is a slight color gradient, with the central region showing a hint of redder hues and the outer regions showing a hint of bluer hues. This suggests that the stellar population is relatively old overall, with some younger stars or regions of ongoing star formation possibly present in the outer parts. There are no signs of any major merger events currently occurring, although a slight asymmetry in the shape might indicate a past interaction or minor disturbance.
