The galaxy presents a largely smooth, elliptical morphology with a bright, concentrated core. There is a gradual decrease in luminosity from the center outwards, indicating a relatively high degree of central stellar density. The galaxy appears relatively isolated, with no obvious signs of major tidal interactions or mergers. Subtle disturbances may be present, but they do not significantly disrupt the overall elliptical structure. The overall color profile suggests a population dominated by older stars, although there appears to be a small amount of star formation ongoing. The object exhibits a roughly round shape.
