The observed galaxy presents as a spiral structure, viewed at a near face-on inclination. Distinct spiral arms are evident, exhibiting a morphology that appears to be well-defined and structured. The arms display a moderate winding, neither tightly wound nor exceptionally loose. Flocculent structures are visible along the spiral arms, suggesting regions of active star formation.

A central bulge is present, exhibiting a yellow/orange hue, indicative of an older stellar population. The bulge appears relatively small in proportion to the overall disk size. The galaxy disk displays a range of color and luminosity, possibly indicating variations in stellar populations and dust content.

There is also a potential minor disturbance in the galaxy's morphology.
