The galaxy presents as an edge-on spiral, with a disk exhibiting a high degree of inclination relative to our line of sight. The central bulge is prominent and appears to be of a rounded morphology. The galaxy has an apparent smooth texture, with no readily discernible spiral arm structure. There is a subtle indication of minor disturbances in the disk, suggesting a possible interaction or past merger event. The color gradients indicate a relatively low star formation rate. The galaxy has a moderate mass. 
