This galaxy exhibits an elliptical morphology, appearing generally smooth and somewhat elongated. The primary light distribution suggests a centrally concentrated bulge, transitioning into a fainter, more diffuse halo. The color profile indicates a redder core, potentially indicating an older stellar population, with a subtle shift towards bluer hues in the outer regions, possibly reflecting some level of ongoing or recent star formation. There is no obvious indication of spiral arm structure or strong tidal distortions, suggesting that it is not currently undergoing a major merger, or a merger has completed. The galaxy appears relatively undisturbed in its overall form.
