The galaxy appears to be a relatively smooth, round object. It exhibits a concentrated central bulge that appears golden in color, likely indicating a population of older stars. The outer regions of the galaxy fade gradually into the background, with little evidence of spiral arms or distinct features. There is no indication of significant tidal disturbance or merging activity based on its morphology. The galaxy's redshift suggests it is at a considerable distance, and the overall color profile suggests relatively low star formation activity.
