The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile exhibits a gradual decrease in intensity from the core outward, suggesting a lack of distinct spiral arms or features. The galaxy's color appears predominantly yellow-orange, indicative of an older stellar population and minimal ongoing star formation. There might be some minor disturbances in the outer regions of the galaxy. The overall morphology suggests a galaxy that is nearing the end of its evolution, with a reduced rate of star formation and a generally relaxed structure.
