The object presents as a spiral galaxy viewed at a slight angle from face-on. Prominent spiral arms extend from a central bulge, exhibiting a tightly wound morphology. The central bulge appears small relative to the overall disk size. The disk displays a mottled texture, suggestive of active star formation regions distributed throughout the spiral arms. The spiral arms appear well-defined, with multiple arms visible. There is no clear indication of a strong bar structure. No major disturbances or ongoing merger activity are readily apparent, although some minor asymmetry in the arm structure hints at potential interactions or internal dynamics. The overall color suggests a mix of stellar populations, with the bulge appearing yellower than the bluer arms.