The galaxy appears to be a spiral galaxy, observed edge-on from our vantage point. There is a clear central bulge which displays a yellowish-orange hue. This suggests an older stellar population within the bulge, with a lower rate of on-going star formation. The galaxy exhibits a flattened disk structure, which extends laterally from the bulge and shows evidence of dust lanes obscuring the starlight within the disk. The disk itself displays bluer regions indicating pockets of active star formation. The overall structure suggests a relatively massive galaxy. There is a slight asymmetry present which could potentially indicate minor tidal interactions or recent merger activity with a much smaller galaxy.