The galaxy presents an elongated morphology with a significant central concentration of light. A fainter, diffuse extension is observed extending from one side of the central region. The color of the galaxy appears predominantly blue, especially in the core, suggesting ongoing or recent star formation activity. The galaxy is relatively small in angular size. The overall shape indicates a possible disturbed or peculiar morphology, potentially due to a past interaction or merger event. The relatively smooth light distribution in the core suggests the presence of an older stellar population as well.
