The galaxy presents as a spiral type, with a well-defined disk structure. Two prominent spiral arms are visible, exhibiting a medium degree of winding. The arms appear somewhat flocculent, displaying clumpy regions suggestive of active star formation. The central bulge is moderately sized, contributing a significant portion of the galaxy's overall luminosity. There is the presence of a bar structure, which appears prominent. The galaxy is viewed at a slight inclination, offering a view that is neither perfectly face-on nor edge-on. There is no sign of any major galaxy merging or disturbance. The galaxy shows characteristics that suggest that a significant amount of star formation is occurring within it. 
