The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated light profile. The core region displays a yellowish-orange hue, suggesting an older stellar population, while the outer regions are a mix of yellow and white, with some hints of blue. There is no visible spiral structure and no obvious dust lanes. The galaxy is quite symmetrical, with an apparent axis ratio of roughly 0.8, indicating it is moderately flattened along one axis. The size is medium, not unusually compact nor overly extended. The color gradient suggests star formation may be low. The absence of significant irregularities indicates it may be relatively undisturbed.
