The galaxy presents as a largely featureless, elliptical morphology. The light profile appears smooth and centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. The galaxy's color is predominantly yellowish-white, suggesting an older stellar population with fewer young, massive stars. There are hints of blue within the galaxy indicating a slightly younger population within it. The overall round appearance, with only minor deviations from perfect symmetry, indicates a relaxed system that is not undergoing any major interactions or recent mergers. There are no obvious dust lanes, spiral arms, or prominent star-forming regions visible within the galaxy at this resolution. The color is relatively uniform across the galaxy. The data suggests a significant mass and moderate star formation rate.
