The galaxy presents as a somewhat elliptical, though nearly round, structure. The central region exhibits a high degree of luminosity, appearing as a bright, concentrated core. This luminosity decreases gradually outward from the center, suggesting a smooth distribution of stars. There is a slight suggestion of a disk-like structure, but no prominent spiral arms or bar features are discernible. The overall color is predominantly yellowish-white, indicating a population of older stars. There are also hints of blueish color, implying that there may be some young, hot stars in the galaxy. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There may be some minor distortions in the outer regions, possibly indicative of recent or ongoing minor interactions or internal activity.
