The galaxy presents as a relatively smooth, elongated structure. It displays an apparent cigar-shaped morphology, lacking prominent spiral arms or a distinct central bulge. The light distribution suggests a fairly uniform stellar population, with a concentration of light toward the center. The color gradient indicates that the central region has a slight yellowish tint, with the outer disk regions appearing bluer. This color difference could be due to the presence of a larger population of older stars in the central region or increased dust extinction. Overall, the galaxy appears undisturbed, exhibiting no major signs of mergers or tidal interactions. Its smooth appearance implies a lack of recent major star-forming events.
