This galaxy exhibits a distinctly elongated, cigar-like morphology. A smooth, centralized bulge region is observed, with a gradual fading of light intensity towards the outer edges of the galaxy. There's a subtle hint of a disk component, though the smooth fraction is dominant. The color profile suggests a higher concentration of older stellar populations. Based on its redshift, this galaxy is likely a significant distance from our own. Despite its distance, no major mergers or disturbances are directly evident, although there may be minor signs of interaction. The overall appearance suggests a system with relatively low star formation activity.
