The galaxy presents a largely smooth morphology, with a high degree of central concentration. It appears nearly circular, showing minimal deviation from a round shape. There is a subtle hint of an extended feature or possible tidal tail to the left, which could indicate some past interaction or disturbance, but it may also just be a artifact. The color profile suggests an older stellar population, dominating with light towards the redder end of the spectrum. Overall, the galaxy seems to be relatively undisturbed, with no obvious signs of major ongoing merging activity, and potentially little star formation.
