The galaxy presents a clear spiral structure. Two distinct spiral arms emanate from a moderately sized central bulge. The winding of the arms appears loose, extending outward in a somewhat open configuration. The arms show some indication of active star formation, suggested by a slightly bluer tint, contrasting with the yellower hue of the central bulge which may be a result of it's older stellar population. The galaxy exhibits an overall flattened shape and a smaller companion galaxy is visible to the right. There appears to be some interaction between the main galaxy and its smaller companion, suggesting that the smaller companion is potentially in the process of merging or has previously merged with the main galaxy. There is a slight asymmetry in the distribution of light throughout the galactic disk.
