The galaxy presents as a spiral type, with a prominent, elongated bar structure crossing its central region. The bar appears quite substantial, possibly composed of older stellar populations given its yellowish-orange hue. The spiral arms are apparent, though somewhat diffuse and not tightly wound. They exhibit a clumpy texture suggestive of active star formation regions interspersed within them. The central bulge is visible, but not overly dominant compared to the disk. Overall the galaxy has a relatively bright disk with a moderate amount of star formation and a clear bar structure.
