The observed galaxy presents as a flattened elliptical morphology. It exhibits a smooth, featureless structure with a gradual increase in luminosity towards the center. The galaxy's color profile shows a predominantly yellowish-red hue, indicative of an older stellar population. There is a potential for a minor dust lane or ring structure, but the resolution limits a clearer assessment. The overall impression is that of a mature, passively evolving galaxy at a moderate redshift.
