The galaxy presents as a flattened, elongated structure, suggesting a disk-like morphology observed at a high inclination. Its central region exhibits a brighter, yellowish-white hue, possibly indicating a concentration of older stellar populations. Fainter, diffuse bluish regions are observed along the edges of the disk, hinting at the presence of younger, hotter stars within spiral arms. A subtle dust lane may be present, bisecting the galaxy's major axis, though the resolution is insufficient to confirm this definitively. There are no obvious signs of recent major mergers. There is some indication of minor tidal disturbances in the disk. Overall, the galaxy appears to be a relatively quiescent system, with ongoing but perhaps subdued star formation activity in the outer regions.
