The galaxy presents as a centrally concentrated, elliptical morphology. The color profile is dominated by redder hues, suggesting an older stellar population and a cessation of significant star formation. The smooth light distribution and lack of any obvious spiral arm structures or dust lanes indicates a morphology likely devoid of significant ongoing star formation. The overall roundness of the galactic form does not suggest major interaction or merger events. The general appearance is consistent with an early-type galaxy at intermediate redshift, likely a massive system.
