The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated, bright central bulge, which suggests a high density of stars. The galaxy displays a yellowish hue, possibly indicating an older stellar population, with lower levels of recent star formation activity. There is minimal visible structure, such as spiral arms or dust lanes. It is generally round, lacking any pronounced asymmetry or tidal features suggesting recent major mergers. There might be some minor distortions in the outer regions, suggesting past or ongoing interactions, but overall, the galaxy appears undisturbed.
