The galaxy presents as a moderately inclined spiral, possibly nearing edge-on orientation. The central bulge appears relatively small and indistinct, showing a smooth, concentrated light distribution. The disk is clearly present, appearing slightly disturbed or warped along its major axis. Evidence of dust lanes are visible, particularly on the near side of the disk where they cause significant obscuration of the starlight. The spiral arms are not well-defined but appear clumpy, indicating regions of active star formation. The overall color suggests a mix of stellar populations, with some bluer regions indicative of younger stars and some redder regions indicative of older stars. The galaxy does not show any obvious signs of a major ongoing merger, but some minor irregularities hint at past interactions or a minor disturbance.
