The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge, which appears relatively small. The winding of the spiral arms appears to be loose, with evidence of ongoing star formation within the arms. The color of the arms appears bluer than the core, indicating a younger stellar population in the arms. The overall appearance suggests that it is currently undergoing active star formation. There appears to be a minor asymmetry or disturbance in the overall structure, potentially indicating a past or ongoing interaction with another galaxy. There is no sign of any dust lanes. The bulge is yellowish.
