The galaxy appears as a flattened elliptical or lenticular system. The central bulge is bright and elongated along its major axis, exhibiting a yellowish hue. Surrounding the bulge is a fainter, bluish disk. The disk appears relatively smooth and featureless, without any discernible spiral arm structure. The outer regions of the galaxy fade into the background, indicating a gradual decrease in stellar density. The overall morphology suggests an evolved system with ongoing or recently ceased star formation. There appears to be minor signs of disturbance, but for the most part, it appears to be a singular galaxy with no mergers.
