The galaxy presents as a disk-shaped structure viewed nearly edge-on.  There is a pronounced central bulge, appearing yellowish-white in color, suggesting an older stellar population. Extending outward from the bulge are fainter, bluish tinged areas. The bluish coloration suggests the presence of younger, hotter stars and ongoing star formation, particularly in the outer regions of the disk. The galaxy exhibits a smooth texture overall with no obvious spiral arm structure or significant signs of recent major merger events. It appears to be a relatively massive galaxy with modest levels of star formation. The orientation and smooth features indicate it could be a lenticular galaxy. The high degree of observation that it is edge-on suggests it is most likely a disk galaxy.
