The object appears to be a spiral galaxy, seen at a high inclination, but not quite edge-on. The disk component exhibits distinct spiral arm structures. These arms appear tightly wound and somewhat fragmented, with noticeable knots of blue light, suggestive of active star formation regions. The central bulge is prominent and appears yellowish-white in color, indicating an older stellar population. The overall light distribution suggests a smaller bulge relative to the size of the disk. There is no obvious sign of strong bar structure in the central region. No major signs of interaction or significant morphological disturbance are readily apparent, though a subtle asymmetry may exist in the outer disk. 
