The galaxy appears to be an elongated, cigar-shaped structure. A central bulge is evident, exhibiting a yellowish-orange hue, possibly indicating an older stellar population. The outer regions of the galaxy appear bluer, hinting at the presence of younger, hotter stars and potential star formation. The galaxy seems relatively smooth in overall appearance, with no immediately obvious signs of major disturbances or ongoing mergers. There is a suggestion of a disk-like structure, although it is not sharply defined.
