The galaxy appears to be a spiral galaxy viewed at a significant inclination, almost edge-on. The central bulge is pronounced, exhibiting a yellowish hue, suggesting an older stellar population. Fainter spiral arms are visible extending outward from the bulge, displaying a bluer color, indicating the presence of younger, hotter stars. These arms appear somewhat flocculent and not as well-defined. There is a faint disk component surrounding the bulge, and indications of dust lanes are present. The galaxy appears to be relatively isolated, and shows no obvious signs of a recent or ongoing major merger event. Based on the color and morphology, the galaxy appears to be experiencing a low rate of star formation.
