The galaxy presents as a spiral type, viewed at a slight angle relative to face-on. Two prominent spiral arms emanate from a bright, moderately sized central bulge. The winding of the spiral arms appears medium. The arm structure is somewhat flocculent and has several breaks and knots, suggesting regions of active star formation. The color gradient across the galaxy indicates a relatively young stellar population, particularly within the spiral arms. The galaxy does not appear to be undergoing any major merging events, though minor disturbances cannot be ruled out. There may be a faint bar feature present, though it is difficult to resolve clearly. Overall, this galaxy exhibits characteristics of a star-forming spiral with ongoing, widespread stellar nurseries.
