The galaxy presents as a spiral type, with a visible disk structure, although some disturbance is also apparent. The spiral arms are well-defined and open, exhibiting a high degree of symmetry, indicative of a developed spiral structure. A bar structure may exist, although this is not definitive based on the image. The central bulge appears to be a moderate size relative to the disk and is smoothly luminous. The disk is not observed to be edge-on. There is visual indication of a possible minor interaction or disturbance, affecting the symmetry of the spiral arms. Overall light distribution indicates the disk has a generally blue spectral signature, while the bulge is slightly redder.
