The galaxy exhibits a prominent disk structure, viewed at an oblique angle. Spiral arms are evident within the disk. A central bulge is present, though it appears relatively small in proportion to the disk. Dust lanes are observed, particularly along the edges. The overall light distribution suggests a classification as a spiral galaxy, likely of type Sb or Sc. The galaxy's shape is significantly elongated, implying a considerable inclination angle relative to our line of sight. The galaxy is not showing any major signs of mergers or major disturbances. The color profile indicates a generally blue hue in the outer regions, indicative of ongoing star formation, while the central region exhibits a yellowish color, potentially suggesting an older stellar population.
