The galaxy presents as a concentrated, ellipsoidal structure. The core region exhibits a bright, relatively uniform yellow-white glow, suggesting an older stellar population. The isophotes appear smooth and regular, tapering off gradually into the surrounding space. There is very little evidence of spiral arm structure or dust lanes, lending credence to a classification as an elliptical galaxy. A very subtle disc may exist, as the ellipticity is quite high, but further observation would be necessary to confirm this. Subtle variations in color, moving from more yellow in the center to more orange at the edges could indicate a difference in star age depending on the distance from the center. No current interactions or mergers are visible.
