The galaxy presents an elongated, cigar-shaped morphology. It exhibits a relatively smooth overall appearance, with a dominant central bulge appearing a yellowish-orange hue. The outer regions appear to be slightly bluer, hinting at the presence of younger stellar populations and ongoing star formation, although at a low rate. There are no clear signs of spiral arms or a well-defined disk structure. Minimal evidence suggests any recent or ongoing merger events, or any significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
