The galaxy presents a primarily face-on orientation with a notable spiral structure. Although not sharply defined, spiral arms are discernible and appear somewhat flocculent in nature. A central bulge is present, appearing relatively small to moderate in size compared to the overall galactic disc. There is evidence of a bar-like structure extending through the central region of the galaxy, although not highly prominent. The overall color of the galaxy is predominantly bluish, suggesting a younger stellar population and ongoing star formation. There are some irregular features within the spiral arms, possibly indicating areas of active star formation or minor disturbances within the galactic disc. The galaxy appears relatively isolated, with no obvious signs of recent major mergers or significant tidal interactions with other galaxies.
