The galaxy presents as a primarily smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a high stellar density, and possibly an active galactic nucleus. The color is predominantly yellow, indicating a population of older stars with lower rates of ongoing star formation. Faint extensions of diffuse light are observed surrounding the central body, possibly a halo of older stars or tidal debris. The galaxy appears relatively undisturbed, with no major signs of recent mergers, although some minor asymmetry cannot be ruled out. The galaxy's overall structure is well-defined, with a gradual decrease in luminosity from the core outwards.
