The galaxy presents as a spiral galaxy. It exhibits a moderate inclination relative to our line of sight. Two distinct spiral arms are visible, and display a medium winding. The central bulge appears small to moderate in size, showing a yellow-white color, indicative of an older stellar population. The spiral arms exhibit a bluer hue, suggesting ongoing star formation. There is evidence of a central bar structure running horizontally through the bulge of the galaxy, contributing to the overall organized spiral structure. There is no clear sign of any major mergers in the galaxy. There is some patchy dust observed in the spiral arms.
