The observed galaxy presents as a spiral structure, exhibiting a relatively low inclination angle relative to the observer's line of sight. It is dominated by tightly wound spiral arms which are clearly evident. The arms display a two-armed morphology. The central bulge appears small relative to the overall disk size. There is no discernable bar feature evident. Overall, there does not seem to be a clear sign of ongoing or recent major mergers. The overall shape of the galaxy appears to show some minor disturbances. 
