The galaxy exhibits a morphology consistent with an elliptical galaxy, appearing largely featureless and smooth in structure. Its shape is somewhat elongated but predominantly round. The galaxy displays a notable concentration of luminosity towards its center, suggesting the presence of a dense galactic nucleus. Coloration appears generally redder, indicative of an older stellar population and diminished rates of current star formation. There is no immediately apparent evidence of significant ongoing merger activity or substantial tidal disturbances affecting the galaxy’s overall morphology.
