This galaxy exhibits a disk-like structure, though it is not perfectly face-on. There is some evidence of spiral arm structure, but they appear somewhat flocculent. The galaxy has a moderate central bulge and the disk exhibits moderate blueness, suggesting ongoing star formation. There may be some minor disturbances, and the overall appearance suggests a transitional state, neither perfectly smooth nor highly disturbed. Its estimated size suggests it is likely a galaxy with a stellar mass around 10^11 solar masses. It likely has moderate levels of star formation.
