The galaxy appears as a moderate-sized, elliptical-like structure with a smooth, concentrated light profile. It exhibits a yellowish-orange hue. The galaxy has a relatively high degree of central concentration. There appears to be little to no evidence of spiral arm structures or significant star formation regions within the observed wavelengths. There are no obvious signs of a major merger event, though a slight asymmetry could indicate minor tidal interactions or disturbances. The object presents a generally smooth, featureless appearance, possibly indicating an older stellar population.
