The galaxy appears to be a spiral galaxy, likely viewed edge-on from our line of sight. It exhibits a flattened, elongated morphology, characteristic of a disk galaxy. There is some indication of a central bulge, but it appears relatively small compared to the overall size of the disk. The galaxy's light profile suggests it is likely experiencing low levels of star formation. The disk appears relatively smooth, suggesting a lack of significant recent merger activity or major tidal disturbances. The galaxy is likely a moderate-mass system.
