The galaxy presents as a spiral type, exhibiting a flattened disk structure with a prominent central bulge. The spiral arms are well-defined, displaying a morphology characterized by distinct winding. These arms extend outwards from the central bulge, tracing a non-uniform pattern across the disk.

The central bulge appears bright and concentrated. The disk shows variations in luminosity, with the spiral arms appearing brighter than the inter-arm regions. There's a hint of a bar-like structure bisecting the bulge, although it doesn't appear to be particularly strong. Overall, the galaxy appears relatively undisturbed, without obvious signs of a major merger event. The outer regions of the disk appear relatively smooth, with the spiral arms gradually fading into the background.
