The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, largely featureless appearance without prominent spiral arms or distinct dust lanes. The light distribution is dominated by an ellipsoidal component, appearing roughly circular. There is a gradual fading of light intensity from the core outwards, suggesting a bulge-dominated morphology. The color profile indicates a population of older stars, inferred from the reddish-yellow hue. There is no indication of active star formation regions within the galaxy's visible extent, and no evidence of a major ongoing merger or tidal disturbance. The galaxy appears relatively undisturbed and isolated, with a symmetric profile indicating that it is relatively relaxed.
