The galaxy presents as a spiral with a bright, moderately sized central bulge. The spiral arms are tightly wound and exhibit a flocculent structure. There is evidence of ongoing star formation within the arms, indicated by bluer regions suggesting the presence of young, hot stars. The central bulge appears relatively smooth. There is a hint of a bar-like structure extending from the center, but it is not very prominent. The galaxy does not appear to be undergoing a major merger or tidal disruption, though some minor disturbances or asymmetries in the outer arms may be present. The overall color suggests a spiral galaxy with a moderate rate of star formation.
