The observed galaxy presents as a relatively compact object. The morphology suggests a mostly smooth structure, with the majority of the light concentrated in a central region, suggestive of a spheroidal galaxy. The concentration of light gradually fades outwards from the center. There is a possible indication of a slight disturbance or asymmetry in the galaxy's outer regions. No well-defined spiral arms or a prominent disk structure are discernible. The main body appears somewhat elliptical in shape, not perfectly circular. The color profile indicates a stronger emission in the green bands, with less in red. Overall, the galaxy appears to be of moderate red shift with possible merger activity, but is mostly smooth. 
