The galaxy presents as a relatively smooth, elongated structure. Its morphology suggests a flattened, cigar-shaped form, with a high degree of ellipticity. The central region appears brighter and more concentrated, exhibiting a yellowish hue. This could indicate an older stellar population dominating the core. Moving outward from the center, a bluer color gradient is noticeable, possibly suggesting the presence of younger, hotter stars in the outer regions. The overall texture lacks prominent spiral arm structures or significant dust lanes, suggesting that it may be an elliptical or lenticular galaxy viewed edge-on. There may be minor irregularities or disturbances in its outer regions, but overall the galaxy is fairly uniform in its distribution of stars and gas. 
