The galaxy presents an elongated, cigar-shaped morphology, with a generally smooth appearance. There is a subtle color gradient across the galaxy, with the central region exhibiting a warmer, reddish-orange hue, possibly indicating a concentration of older stellar populations or dust. The outer regions of the galaxy appear to be less concentrated, with a fainter and bluer glow that could be caused by younger stars forming. There are no clear signs of spiral arms or significant irregularities or tidal tails, suggesting a relatively undisturbed system. Overall, the galaxy seems to be a mature system.
