The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth with a high degree of central concentration. There is a subtle color gradient visible, trending from a yellowish-white core to slightly bluer edges. There is no strong evidence of spiral arm structure, and the outer regions of the galaxy fade gradually into the background. No major disturbances are visible in the galaxy's form, though very minor signs of past interactions or internal activity cannot be ruled out based on this image alone.
