The galaxy presents as a spiral, possessing a morphology that suggests active star formation. The spiral arms are relatively tightly wound around a central bulge of moderate size. The bulge exhibits a yellowish hue, indicative of an older stellar population. Patches of bluer light are distributed throughout the disk, likely regions of ongoing star formation within the spiral arms. Faint suggestion of two main spiral arms with a large fraction reporting 2 spiral arms. There appears to be no strong bar structure, or any bar at all. Overall, there are no obvious signs of major merging activity, although the galaxy could be experiencing a minor disturbance.