The galaxy exhibits a distinct spiral morphology, characterized by loosely wound arms. Two spiral arms are clearly discernable. The central bulge appears relatively small compared to the overall disk size. The galaxy displays a prominent disk structure, viewed nearly face-on, and does not present an edge-on orientation. There is no visual evidence of a strong bar feature crossing the galactic nucleus, nor is there significant tidal disruption or merging activity. The color suggests active star formation. The galaxy shows faint indications of possible minor disturbances in its symmetry, but appears, for the most part, unperturbed.
