The object appears to be a galaxy, likely an edge-on or nearly edge-on spiral. Its disk is clearly visible, exhibiting a high degree of dust lane obscuration. The central bulge is prominent and has a rounded morphology. No strong evidence of a classical spiral arm structure is apparent within the disk, suggesting a more homogenous stellar population. The overall color index indicates a redder galaxy, which could mean that it is older, or the light is being shifted toward the red end of the spectrum from its velocity (redshifted). Faint signs of possible tidal features or minor disturbances can be observed within the image, but more data are needed for verification. It appears to be a substantial galaxy.
