The galaxy appears as a flattened, disk-like structure, presenting an edge-on or highly inclined orientation relative to our line of sight. The central region exhibits a bright, concentrated luminosity, suggesting the presence of a prominent galactic nucleus or bulge. Fainter, extended emission can be observed tracing the disk, which appears to be relatively thin and uniform. The galaxy displays no obvious signs of strong spiral arm structures or intense star formation regions. The overall color appears consistent, without significant color gradients or irregularities, pointing towards an older stellar population. There is a subtle asymmetry in the galactic disk, hinting at possible past interactions.
