The galaxy presents an elongated, somewhat irregular morphology. Its light profile appears relatively smooth across the majority of its extent, exhibiting a concentration of light towards the central region. There is evidence of what seems to be a disk, but it is not sharply defined. The galaxy exhibits a blueish hue, which could indicate recent or ongoing star formation. Signs of minor disturbances, such as tidal features, are weakly present, possibly indicating a past interaction or merger event.
