The galaxy presents as a relatively small, faint object. It is a disk galaxy seen nearly edge-on from our vantage point. There is evidence of a central bulge component that appears somewhat rounded. There are no strong signs of active merging or major disturbances, though some minor peculiarities in the disk morphology cannot be ruled out. The galaxy is generally smooth in appearance, lacking distinct spiral arm structures or prominent star-forming regions. Its color indices suggest a moderate redshift and a relatively low rate of star formation. The overall characteristics suggest a galaxy that is primarily composed of older stellar populations.
