The observed galaxy presents as a relatively small, edge-on spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, rounded morphology. The disk is observed almost perfectly edge-on, with a high degree of flattening. There is no clear indication of spiral arm structure, likely due to the edge-on orientation. The overall color suggests an older stellar population, potentially with a lower rate of on-going star formation. No significant tidal features or signs of recent merging activity are apparent. 
