The galaxy presents as a spiral type with a discernible disk structure. The spiral arms are prominent, with a tightly wound morphology. While there is no strong central bar feature visible, a weak bar may be present.

The bulge component appears relatively small to moderate in size. Star forming regions are apparent within the spiral arms. There are some signs of minor interaction or disturbances in the overall morphology, possibly indicative of past or ongoing gravitational interaction. The overall appearance of the galaxy suggests a well-defined spiral structure with regions of ongoing star formation.
