The galaxy presents as a centrally concentrated, relatively smooth object, exhibiting a flattened, elliptical morphology. The core appears bright and somewhat blue-white in color, suggesting a population of hotter, younger stars or possible active galactic nucleus activity. The light gradually fades as it extends outward from the core, transitioning toward redder hues in the outer regions. The smooth profile suggests a relatively evolved system with minimal recent mergers or major disturbances. Faint hints of extended structure or a very subtle disc-like component are tentatively observed along the major axis. No strong spiral arm features or distinct dust lanes are apparent. The overall color profile suggests the presence of both young and old stellar populations, with the older, redder stars dominating the outer regions.
