The galaxy presents a spiral morphology, exhibiting well-defined spiral arms emanating from a central bulge. The winding of the spiral arms appears moderately compact. A slight bar-like structure seems to bisect the bulge. The bulge itself is prominent, showing a moderate size relative to the overall galactic disk. There is evidence of a relatively smooth disk. Concerning disturbances to the galaxy's form, I observe the presence of features indicating a minor gravitational disturbance, possibly due to a past or ongoing interaction. There is also a suggestion of more significant disruption.
