The galaxy presents a prominent, bright central bulge. It is surrounded by a disk-like structure that appears to be populated with spiral arms, though these are somewhat tightly wound and difficult to fully resolve. The galaxy is not viewed edge-on, but at a slight angle, allowing for observation of spiral features. There may be a weak bar structure in the center. The galaxy shows a generally smooth appearance with only minor disturbances if any. It appears to be an example of a spiral galaxy with active star formation. The presence of the tightly wound spiral arms could suggest a higher degree of differential rotation.