The galaxy presents a complex morphology. Its light profile suggests an elliptical galaxy with a relatively smooth distribution of light. However, there are indications of a more complex structure, possibly involving a merging event or tidal interactions. The galaxy's central region exhibits a concentrated luminosity. Faint extensions are visible, potentially representing tidal tails or debris from a past interaction. The galaxy exhibits a red color, suggesting that it is primarily composed of older stellar populations. Patches of bluer light are also visible within the galaxy, which may indicate regions of more recent star formation.
