The galaxy presents as a centrally concentrated object with an elliptical morphology. A dominant bulge component is apparent, displaying a yellowish-white hue, suggesting an older stellar population. The outer regions exhibit a fainter, bluish color, hinting at the presence of some younger stars and possibly ongoing, albeit subdued, star formation. The overall structure appears relatively smooth and undisturbed. There's no obvious presence of spiral arms or a well-defined disk. The galaxy seems to be more spheroidal in shape rather than a flattened disk-like galaxy. Minor asymmetries may be present in the outer regions, but are difficult to discern without further analysis. There are no clear signs of tidal tails or distortions, which indicates no recent major merger events.
