The galaxy presents as a spiral type, though at an angle which makes it difficult to fully ascertain its morphology. There's likely a weak bar structure present in the center. The spiral arms are tightly wound around a moderately sized bulge. There appear to be at least two prominent spiral arms extending from the central region. The galaxy exhibits a moderate amount of star formation. There is a prominent disk with a relatively smooth appearance. There is a lack of any significant tidal disturbances suggesting it is isolated.
