This galaxy exhibits a clear spiral structure. Two prominent spiral arms emanate from a central bulge, displaying a moderate winding. The arms are well-defined, appearing somewhat flocculent with localized areas of brighter emission that suggests active star formation regions. The central bulge is relatively bright and elongated, indicating a bar-shaped structure. Overall, the galaxy appears relatively undisturbed with no obvious signs of a major merger, though there may be minor asymmetries within the arm structure suggesting potential past interactions. The disk of the galaxy is viewed at an angle that is far from edge-on. The light from the galaxy skews toward the red end of the spectrum.