The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth and diffuse morphology. There's a noticeable central bulge that appears brighter than the surrounding disk, though the disk itself shows subtle variations in luminosity. The galaxy's color gradient suggests some level of stellar population variation, with the central region potentially exhibiting a slightly redder hue compared to the outer regions. Overall, the galaxy displays a relatively high degree of symmetry, without any obvious signs of major disturbances or tidal features, with a few low-level disturbances. It's relatively round, but not completely spherical. The redshift indicates that the galaxy is at a modest cosmological distance. The light appears bluer in the center of the object. The size of the object is reasonably consistent with what is expected from a galaxy at this distance. 
