The galaxy presents as a barred spiral type, with a discernable central bar structure. Prominent spiral arms extend from the ends of the bar. These arms display a clumpy, discontinuous morphology characterized by numerous regions of enhanced blue emission. This suggests ongoing or recent star formation activity within these spiral arms. The central bulge appears relatively small. The disk is viewed at a slight angle, not quite edge-on, allowing for observation of spiral structure. Evidence of significant disturbance is observed in the galaxy. Some of the spiral arms look diffuse, suggesting a recent interaction.
