The galaxy presents as a disk galaxy oriented approximately edge-on, with a moderate bulge. Spiral arm structures are evident, though somewhat tightly wound and not highly contrasted against the disk. A prominent bar feature crosses the central region of the galaxy. The bulge appears yellowish in color, suggesting an older stellar population, whereas the disk exhibits regions of bluer hues, indicative of more recent or ongoing star formation. The overall morphology suggests a system that has undergone some degree of dynamical evolution, potentially with past or ongoing interactions that have influenced its structure. No signs of a major merger are apparent. 
