The galaxy exhibits a spiral structure with tightly wound arms emanating from a central bulge. The arms show evidence of active star formation, indicated by the presence of blue-ish regions. The bulge appears relatively large and prominent, suggesting the presence of an older stellar population that is more yellow-red in color. Overall, the galaxy appears to be relatively face-on, allowing for clear observation of the spiral arm structure, which is faint. There are distinct dust lanes visible within the spiral arms and the galaxy is somewhat elliptical in shape.
