The galaxy presents a largely smooth, elliptical morphology. Its light profile exhibits a centrally concentrated bulge, which dominates the overall luminosity. There is a faint, diffuse halo surrounding the central region, suggesting a gradual decline in stellar density with increasing radius. The galaxy appears relatively isolated, showing no obvious signs of recent major merger activity. The overall color index suggests a population of older stars with moderate levels of on-going star formation activity. There are no prominent features or dust lanes visible within the galaxy's structure.
