The observed galaxy presents as a flattened, elongated structure, indicative of a disk galaxy viewed edge-on. The dust lane is subtly visible as a dark band that bisects the galactic plane, obscuring light from the galactic bulge and disk stars behind it. The galactic bulge appears relatively small, with a somewhat boxy shape. There is no prominent bar structure visible. The overall color distribution suggests a mix of stellar populations, with some areas appearing bluer, possibly indicating regions of recent star formation. No tidal tails or obvious signs of interaction with other galaxies are apparent. The galaxy appears relatively isolated, residing within a relatively empty field.
