The galaxy presents as a spiral, exhibiting a prominent disk structure. The spiral arms appear to be well-defined, tracing a path from the central bulge outwards. These arms are wound loosely around the central region. The central bulge of the galaxy is moderate in size and displays a smooth, concentrated luminosity profile, indicating a significant population of older stars. There may be a slight asymmetry or distortion in the overall structure, suggesting past or ongoing minor gravitational interactions. The presence of star-forming regions is implied by the slightly uneven coloration of the arms. The galaxy's morphology indicates a lack of a significant central bar.
