The galaxy appears as an edge-on spiral, exhibiting a clear disk structure. The central bulge is prominent and appears largely spheroidal. There's a moderate amount of dust obscuring the central regions of the galaxy. The overall color gradient suggests a relatively evolved stellar population, with a redder hue throughout the disk and bulge, although some bluer regions might indicate areas of recent or ongoing star formation. No significant tidal features or major disturbances are obviously visible, suggesting it is not undergoing a major merger. Faint, possibly asymmetric features in the halo could indicate minor interactions or past disturbances.