The galaxy presents as a slightly elongated spiral structure, viewed at an oblique angle, not quite edge-on but not fully face-on. There is a noticeable central bulge region, exhibiting a smooth, concentrated luminosity, while the surrounding disc shows subtle spiral arm features. The arms appear somewhat loosely wound and patchy in luminosity, indicating areas of differing stellar density or star formation activity. Overall the galaxy appears more blue in color, which could be indicative of ongoing or recent star formation. The galaxy does not show any strong signs of tidal disturbances or recent major merger events, though some minor asymmetries or irregularities in the outer disc may hint at past interactions. The disk extends noticeably beyond the central bulge and is surrounded by a faint halo. The galaxy displays a general overall structure indicative of a spiral galaxy transitioning into a lenticular type, where star formation is slowing, and the spiral arms are becoming more diffuse.
