The galaxy presents as an elliptical or lenticular type, appearing largely smooth and featureless. There is a subtle elongation, suggesting a shape that deviates slightly from perfectly spherical but not severely so. The galaxy exhibits a color gradient; its core region appears more yellowish, suggesting an older stellar population, while the outer regions show a slight bluish tint indicating the presence of some younger, hotter stars, although this is not pronounced. There is no obvious evidence of spiral arms or a prominent disk structure. The morphology suggests a system that has undergone significant evolution, potentially having exhausted much of its gas supply for star formation. There may be some minor tidal disturbances, but the galaxy appears generally isolated. The overall impression is of a relatively massive, passively evolving galaxy at a moderate redshift.
