The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a galactic bulge. Dust lanes appear prominent along the galactic plane, obscuring and reddening the light from stars behind them. No spiral arm structure or distinct features are visible, implying a smooth morphology. The outer regions of the disk gradually fade into the background, indicating a decreasing stellar density with radial distance. There is no apparent sign of any major mergers or tidal disturbances. The bulge morphology is largely undetected, but what can be seen points to a typical rounded shape. The galaxy's stellar population is predominantly mature, exhibiting a low specific star formation rate.
