The galaxy presents as a face-on spiral galaxy with a prominent central bulge exhibiting a yellowish hue. The spiral arms are well-defined and extend outwards from the central bulge. They appear to be relatively tightly wound. The color of the arms shows distinct bluish concentrations, suggestive of ongoing star formation. The galaxy displays an overall moderate degree of central concentration. There is no obvious evidence of a strong bar structure. No major merger events are apparent, although some minor irregularities in the outer regions of the disk could suggest minor interactions.
