The galaxy presents as an elongated, somewhat cigar-shaped object with a noticeable color gradient. A central bulge or core region exhibits a yellow-orange hue, suggesting a population of older stars. This area appears relatively smooth and featureless. Extending outward from this core is a disk-like structure. One section shows blue-green tinges which likely indicates regions of active star formation, and therefore, the presence of younger, hotter stars. There appear to be areas of minor dust and gas present but no major disturbances are visible. The overall structure implies an early stage of galaxy evolution with ongoing, yet not vigorous, star formation.
