The galaxy presents a largely featureless, elliptical morphology. It displays a bright, concentrated central bulge that dominates the overall luminosity. The light smoothly decreases outward from the core with a gentle gradient. No distinct spiral arm structures or prominent dust lanes are discernible in the image. The galaxy exhibits a slight ellipticity, appearing somewhat flattened along its minor axis. There are no obvious signs of recent or ongoing major mergers. The color profile suggests a population of older stars with a redder hue, particularly in the central region. The outer regions appear slightly bluer, possibly indicating the presence of younger stellar populations, though these are not readily apparent. Overall, the galaxy appears to be a relatively relaxed, evolved system.
