The galaxy appears to be a spiral galaxy, viewed nearly edge-on. There is a concentrated central bulge that seems relatively smooth. The galaxy has a disk with indications of some features, but it lacks defined spiral arm structure. The light from the disk is diffuse, indicative of some dust obscuration, but the disk seems to be generally thin. There may be a slight tidal feature or minor disturbance on the disk. The galaxy is bright, exhibiting a prominent red glow relative to the blue. This indicates an older stellar population and comparatively low recent star formation activity, suggesting it is relatively evolved and likely a massive system. 
