The galaxy exhibits a smooth, elliptical morphology, with a moderate degree of elongation. The light distribution appears relatively uniform across the galactic body, with a concentration toward the center, suggesting a prominent galactic nucleus. There's a gradual decrease in luminosity from the core outwards, with no discernible spiral arm structure or distinct features, though a subtle hint of disk structure may be present. The color profile shows a tendency towards redder hues, indicative of an older stellar population and lower levels of current star formation activity. There is no obvious evidence of tidal disturbances or ongoing major mergers.
