The galaxy presents as a predominantly smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, suggesting a high stellar density or possible active galactic nucleus. There is a notable radial gradient in luminosity, decreasing from the core outwards, indicative of the stellar distribution within the galactic body. While appearing mostly uniform in structure, closer inspection suggests a subtle elongation. There is no distinct spiral arm structure, no prominent dust lanes, or signs of significant recent mergers or tidal disturbances visible in this image, although very faint disturbances are still present. Overall, the galaxy appears to be relatively mature and well-formed.
