The galaxy presents a morphology consistent with a spiral galaxy. The central bulge appears prominent and exhibits a yellowish hue, potentially indicating an older stellar population. The spiral arms are somewhat flocculent, displaying a patchy distribution of star formation regions. These regions are characterized by a bluer color, suggesting the presence of younger, hotter stars. The winding of the spiral arms appears to be moderately tight. There is a suggestion of one dominant spiral arm, although fainter features may indicate a multi-armed structure. The overall disk appears relatively face-on. There is also a slight asymmetry, potentially resulting from an ongoing interaction or merger event. The galaxy is otherwise considered undisturbed. 
