The observed galaxy presents as an ellipsoidal structure, appearing smooth and relatively featureless. The light distribution exhibits a concentration towards the center, with a gradual decrease in intensity towards the periphery, consistent with a spheroidal morphology. The galaxy is subtly elongated, deviating slightly from a perfectly circular shape. No prominent spiral arms or distinct disk-like structures are discernible. There is a slight asymmetry, but no major or minor disturbances are observed. The galaxy's central region is noticeably more luminous with a reddish hue, potentially indicating an older stellar population. A faint yellow glow is observed around the core of the galaxy.
