The galaxy appears as a flattened, elongated structure, possibly a disk galaxy viewed at a high inclination. Its central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar population or active galactic nucleus. The overall color profile indicates a mixture of stellar populations, with bluer hues in the outer regions potentially indicating ongoing star formation and relatively younger stars.  The galaxy seems relatively smooth in overall structure, with a slight tapering off toward the edges of the disk.  The shape appears highly elongated, approaching a cigar-like or needle-like appearance. The galaxy does not appear to display any major interactions or merger events. A minor asymmetry or disturbance cannot be ruled out based on the image.
