The galaxy presents as a spiral structure with a moderately sized bulge, contributing significantly to the overall light profile. The spiral arms are well-defined and exhibit a two-armed morphology, displaying a medium winding. The central region appears relatively smooth and bright, suggesting a concentration of older stellar populations. The disk is viewed nearly face-on, allowing for the spiral structure to be clearly observed. There is no major distortion, but there does seem to be some minor disturbance within the spiral structure. The galaxy exhibits a clear color gradient, transitioning from bluer hues in the outer disk to redder tones towards the central bulge. 
