The galaxy presents as a spiral type, exhibiting a distinct disk structure. Two prominent spiral arms are clearly visible, loosely wound around the central bulge. The galaxy appears to be relatively face-on, allowing for a clear view of its spiral structure. A small bar feature seems present in the central region. The bulge size appears moderate relative to the overall disk. There are indications of minor disturbances, possibly suggestive of tidal interactions or a past minor merger event. The disk exhibits a relatively smooth appearance with no edge-on dust lanes readily visible. The galaxy shows signs of ongoing star formation, which is distributed throughout the spiral arms.
