The galaxy presents an elliptical morphology, exhibiting a relatively smooth light distribution with minimal discernible substructure. The central region displays a concentrated, bright core, suggesting a high stellar density. The galaxy's overall color index appears to be redder, hinting at an older stellar population and a lower rate of on-going star formation. It is elongated, but nearly rounded. No obvious signs of tidal disturbances or major mergers are apparent, although a slight asymmetry might indicate minor interaction. The galaxy's size is consistent with that of a typical galaxy at its estimated redshift.
