The galaxy presents as a spiral type, exhibiting a flattened, disk-like structure. There is evidence of spiral arm morphology, though the arms appear somewhat flocculent and not as well-defined across the entire disk. A central bulge is readily apparent, exhibiting a yellowish hue, suggestive of an older stellar population. The disk displays a bluer color, indicative of younger stars and regions of active star formation. The galaxy shows a moderate inclination relative to our line of sight, preventing a completely face-on or edge-on view. No strong bar structure is obviously visible traversing the central bulge. There does not appear to be any significant morphological distortion or signs of ongoing major merger events. The disk appears relatively undisturbed.
