The galaxy presents as a spiral type, observed at a near face-on orientation. The central bulge appears substantial, exhibiting a moderate concentration of light. Two prominent spiral arms are visible, displaying a relatively tightly wound morphology. Star formation appears to be actively occurring within the spiral arms. There may be a weak bar structure present, but not dominant. No major signs of galactic merging or significant disturbances are evident. Overall, this galaxy seems to be a relatively unperturbed spiral galaxy with ongoing star formation in its spiral arms.
