The galaxy presents as a spiral type, exhibiting a prominent disk structure. Two well-defined spiral arms emanate from the central region, tracing a relatively coherent pattern. A central bulge is clearly visible, exhibiting a moderate size compared to the overall disk. Within the disk, the spiral arms reveal variations in luminosity and color, possibly indicating differing stellar populations or dust lane presence. The overall winding of the spiral arms appears intermediate. There is no obvious major ongoing merging event.
