The galaxy presents a distinct disk morphology, with a notable spiral structure. The spiral arms are somewhat flocculent and loosely wound. There is evidence of active star formation within the arms, indicated by the presence of blue-tinted regions. A prominent central bulge is observed, exhibiting a moderate size relative to the disk. While no strong bar structure is readily apparent, there may be a hint of a weak bar or oval distortion. The galaxy appears relatively isolated, without any obvious signs of a major merger event, though some minor disturbances or interactions cannot be ruled out. The overall color suggests a population mix of both young, blue stars and older, redder stars. The galaxy is resolved, indicating it is relatively nearby.
