The galaxy exhibits a distinct spiral structure with two prominent arms. These arms are loosely wound, extending outwards from a central bulge. A bar-shaped structure is present within the central region, displaying a moderate degree of prominence. The bulge size appears moderate relative to the galactic disk. The disk itself presents a relatively smooth appearance. The color gradients suggest active star formation regions within the spiral arms, exhibiting bluer hues, while the central bulge shows a shift towards redder colors, possibly indicative of an older stellar population. There are no indications of major disturbances or ongoing merger events.
