The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a significant stellar population density. The light distribution is somewhat uniform, decreasing gradually from the center outwards with a slight elongation. There are no prominent spiral arms or obvious dust lanes visible in this image. The overall color is indicative of an older stellar population, with a possible small amount of on-going star formation. There's no apparent presence of any active galactic nucleus.
