The galaxy presents a morphology consistent with a spiral type, although the arms appear somewhat flocculent. The central bulge is relatively bright, and the overall orientation is nearly face-on. The spiral structure seems to exhibit a tight winding pattern. There's a subtle hint of asymmetry within the disk, though there are no significant indications of ongoing major merger activity. The overall color of the galaxy suggests a relatively low rate of star formation, indicated by the presence of redder regions. Based on these observations, it is suggested that this galaxy is a spiral that could potentially be an intermediate spiral such as an SAB.