The galaxy presents as a spiral type. It exhibits a well-defined structure, with prominent spiral arms emanating from a central bulge region. The spiral arms are tightly wound, suggesting a Sa or Sb morphological classification. The galaxy possesses a bar structure running through the central region, spanning a significant portion of the galactic disk. The bulge appears moderate in size relative to the disk. There are more than four apparent spiral arms. There is no indication of a major merger, but some minor disturbances appear to be present within the structure. There are hints of active star formation regions within the spiral arms.
