The galaxy presents as a spiral galaxy, seen at an angle, but not fully edge-on. There is evidence of spiral arm structure, with some indication of ongoing star formation. The central bulge appears moderate in size relative to the disk. The galaxy exhibits a blue hue, suggesting the presence of younger stellar populations, and a relatively low rate of star formation. There is no clear sign of a strong central bar. The overall structure indicates minimal signs of major merging activity, although some minor disturbances might be present. The galaxy is neither perfectly smooth nor particularly disturbed, existing somewhere in between these two extremes.
