The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth in texture, lacking prominent spiral arms or significant morphological disturbances. The central region exhibits a concentrated brightness, possibly indicating a bulge. Fainter, diffuse light extends outwards from the center, creating a flattened, disk-like appearance. There is a slight color gradient noticeable, with the inner regions trending towards bluer hues and the outer edges showing a hint of redder tones. This subtle color variation suggests potential differences in stellar populations or dust content across the galaxy. Overall, the galaxy seems to be relatively isolated and undisturbed, with no clear signs of ongoing mergers or major interactions.
