The galaxy presents as a spiral, viewed at an oblique angle. Prominent spiral arms are visible, exhibiting a tightly wound structure. The arms display a mottled texture, indicative of active star formation regions. The central bulge appears relatively small and moderately bright, fading into the surrounding disk. A weak bar structure may be present, subtly elongating the central region. The galaxy's disk shows a slight warp, hinting at potential gravitational interactions or internal dynamical processes. The color gradient suggests a radial profile of stellar populations, with bluer colors dominating the outer arms, potentially indicating younger stars, and redder hues concentrated in the bulge. No major merging activity is immediately apparent, but there are suggestions of minor disturbances in the outer disk.
