The galaxy appears as a moderately bright, diffuse object with an overall elliptical morphology. The light distribution suggests a relatively smooth structure, potentially indicating an older stellar population. Color gradients are present, with a yellowish hue dominating the central region, possibly indicative of a higher concentration of evolved stars. The outer regions exhibit a slightly bluer tint, which may be due to the presence of younger stars or a lower concentration of dust. There is no obvious indication of spiral arms or a bar structure. The shape appears slightly elongated rather than perfectly circular. The galaxy does not appear to be undergoing any major merging activity, though there could be some minor tidal disturbances. The overall appearance suggests this is likely an elliptical galaxy at moderate redshift.
