The galaxy presents an elliptical morphology, elongated along a discernible axis. Its core exhibits a concentrated luminosity, suggesting a high stellar density within the central region. The light distribution gradually diminishes from the core outwards, forming a smooth, diffused halo. Faint bluish tones are observed in the outer regions of the galaxy suggesting the presence of younger stellar populations. A slight asymmetry is visible in the distribution of light within the galactic halo.
