The galaxy is a disk galaxy, viewed nearly edge-on from our perspective. The central bulge is prominent and appears to be primarily composed of older stellar populations, indicated by its yellowish-white color. There is little to no indication of spiral arm structure or clumpy star formation regions, suggesting a relatively smooth disk. The disk itself appears elongated and thin, with a relatively high degree of flattening. There is no visual evidence of any major ongoing mergers or tidal disturbances and the disk morphology is fairly smooth, although there might be some minor irregularities in the disk’s outer regions. The central bulge appears rounded and somewhat symmetric. Overall, the galaxy appears to be a relatively quiescent disk galaxy with a significant bulge component. The galaxy shows the effects of redshift, causing its intrinsic luminosity to appear dimmer.