The galaxy presents a generally smooth morphology, appearing cigar-shaped with a significantly elongated structure. It shows an overall smooth form but does exhibit subtle features disrupting its smoothness. Color gradients are apparent, with a concentration of yellowish-orange hues in the central bulge region. Progressing outwards, the color subtly transitions towards bluer tones. This color variation could indicate different stellar populations or dust distributions within the galaxy. Indications of minor disturbances are present. No signs of a spiral structure are immediately evident.
