The galaxy presents as a moderately inclined, disk-like structure. The overall morphology appears relatively smooth, with a bright central bulge region. The disk shows a subtle bluing, suggesting ongoing star formation, although the arms are not well defined. The shape is moderately elliptical, and it is neither perfectly round nor particularly elongated. There are no obvious signs of a major ongoing merger or significant tidal disturbances, though subtle asymmetries could indicate a past interaction or minor disturbance. Based on color index, there appears to be relatively more blue light emitted from the galaxy than red.
