The galaxy appears to be a spiral type, characterized by a prominent disk structure. The spiral arms are tightly wound and show a flocculent morphology, with some difficulty in discerning a clear arm count. A moderate bulge is present, exhibiting a yellow-white color indicative of an older stellar population. The disk shows regions of blue hue suggesting on-going star formation. The galaxy shows no significant signs of interaction with another galaxy, although a faint disruption in the disk's symmetry cannot be ruled out. The disk is oriented at an angle to our line of sight, but is not completely edge-on. There is evidence of a bar structure that passes through the bulge.