The galaxy appears to be a relatively smooth, elliptical galaxy. Its shape is quite rounded, with no obvious distortions or tidal features to indicate any ongoing or recent major merger events. The galaxy exhibits a concentrated central bulge, and the overall color suggests an older stellar population, though there is subtle color variation that could reflect some star formation. There are no clear signs of a prominent disk structure, but there may be some slight indications of spiral arms or subtle disk-like features. The color gradient may indicate spatial variation in its stellar populations or dust content. The galaxy's overall morphology is consistent with a lack of active star formation and an evolved stellar population.
