The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. It exhibits well-defined spiral arms emanating from a bright, yellowish central bulge. The spiral arms show a tightly wound structure. The color of the arms appears bluish, suggesting a population of younger, hotter stars. There is a prominent bar structure visible extending from the central bulge. The overall morphology suggests a galaxy undergoing active star formation. There is no indication of a major merger. The bulge is relatively small in size compared to the disk. The galaxy exhibits 3 or more discernible spiral arms.
