The galaxy appears as a single, relatively smooth object. It is elongated in shape, exhibiting a roughly cigar-shaped morphology. The central region shows a concentration of light, suggesting a well-defined galactic nucleus or bulge. The galaxy displays a color gradient from the center outwards, transitioning from a yellow-orange core to a slightly greener outer region. This could be due to differing stellar populations or dust content within the galaxy. There is no clear evidence of strong spiral arm structure or other significant features. It appears largely undisturbed, with no obvious signs of an ongoing major merger, though some minor gravitational interactions cannot be ruled out based on this image alone.
