The galaxy appears to be a relatively smooth, elliptical-like structure. There is a concentrated central bulge with a gradual decrease in luminosity moving outwards. The overall shape is largely round with only minor deviations from a perfectly circular form. I do not observe any spiral arm structures or dust lanes within this image. The color profile displays a dominance of redder and yellower wavelengths in the central regions, potentially suggesting an older stellar population. I do not see any indications of active merging events or substantial tidal disturbances. The galaxy is slightly brighter in the r band than the g band, but the z band brightness is less than the r band.