The observed galaxy presents as a spiral type, oriented approximately edge-on relative to our line of sight. A prominent central bulge is visible, displaying a yellowish hue indicative of an older stellar population. Faint spiral arms extend from this bulge, though their definition is somewhat obscured by the edge-on perspective and moderate redshift. These arms exhibit a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. The dust lanes are subtle but present, contributing to the galaxy's overall structure. The disk appears generally smooth, with no obvious signs of major disturbances or ongoing mergers. The spiral arms appear relatively tightly wound.
