The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears relatively smooth in overall structure, lacking prominent spiral arms or significant clumpy star-forming regions. The color gradient suggests a concentration of older stellar populations in the central bulge, indicated by the more reddish-yellow hue. The outer regions of the galaxy appear slightly bluer, implying the presence of a younger stellar population, or possibly a lower metallicity interstellar medium, though this is subtle. There may be some slight tidal disturbances or signs of a minor interaction.
