This galaxy presents a predominantly disk-like morphology, exhibiting a moderate inclination relative to our line of sight. Evidence for spiral arm structure is apparent, though the arms appear somewhat flocculent and lack well-defined edges. A central bulge is present, appearing relatively small in proportion to the overall galactic disk. The bulge has a yellowish hue which likely indicates an older stellar population. The disk shows a more bluish color, indicative of ongoing star formation. There do not appear to be any signs of a major merger, though there may be some minor disturbance to the galaxy's overall morphology. Dust lanes may be present in the disk, obscuring some of the starlight. The galaxy is well-defined and elliptical in shape.
