The galaxy presents as a spiral type, viewed at an angle that is close to face-on. It exhibits a distinct central bulge that appears moderately bright and yellowish, suggesting an older stellar population concentrated in the core.

Spiral arms are clearly visible, extending outwards from the central bulge. They appear relatively tightly wound, tracing a multi-armed structure. The arms are somewhat clumpy, indicating regions of active star formation. The arms are blueish, suggesting populations of younger, hotter stars within these regions.

There is no apparent strong central bar feature, but some elongation may be present. The overall morphology suggests a relatively undisturbed structure, with no signs of major ongoing mergers, although some minor perturbations or interactions cannot be ruled out from this image alone. 
