The galaxy presents as a centrally concentrated, elliptical structure with a smooth light distribution. The core region exhibits a bright, diffuse glow, suggesting a high stellar density. The isophotes appear generally smooth and evenly distributed, lacking any distinct spiral arms or bar features. There's a slight elongation in the morphology, with an apparent axis ratio suggesting an E4 to E6 classification on the Hubble sequence. The galaxy exhibits a moderate redshift. The system has a low star formation rate. There are no signs of significant recent merger events, and it appears relatively undisturbed.
