This galaxy presents a disk-like morphology, seemingly viewed edge-on from our vantage point. There is evidence of structure within the disk. A prominent central bulge is observed. Indications of ongoing or recent star formation are present, suggested by bluer regions within the disk, though the overall color is relatively red. This suggests a galaxy dominated by an older stellar population, but with pockets of younger, hotter stars. No significant merger events are visible, although there is some minor disturbance in the galaxy's overall morphology. The galaxy appears relatively isolated.