The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggesting an older stellar population. The outer regions fade gradually into the background, displaying a redder color, which could indicate dust obscuration or a difference in stellar population age compared to the core. No prominent spiral arms or distinct features such as star-forming regions are readily apparent. The overall structure appears relatively undisturbed, lacking visual signs of recent major mergers or tidal interactions. The galaxy exhibits a somewhat flattened shape, falling somewhere between round and elongated. There are no apparent signs of an active galactic nucleus based on the image.
