The galaxy presents as a largely featureless spheroid, displaying a smooth light distribution suggestive of an elliptical morphology. The core exhibits high luminosity, indicating a concentrated stellar population and/or active galactic nucleus. Moving outwards, the galaxy's light gradually diminishes, with no prominent spiral arms or distinct morphological features discernible. The overall color appears slightly redder, which is consistent with an older stellar population and lower star formation rate. There appears to be no signs of a major merger or tidal disturbances.
