The galaxy presents a moderately concentrated light profile. The central region exhibits a brighter, more intensely colored core, surrounded by a less concentrated halo of light. There is a degree of asymmetry in the distribution of light, with suggestions of disturbances in the outer regions. These disturbances could possibly be caused by a past interaction with another galaxy. There is a hint of faint extended features emerging from the main body. The galaxy displays a color gradient, appearing bluer in its central regions and shifting towards redder hues in the outer parts of the halo.
