The galaxy presents a generally smooth morphology. The central region exhibits a high surface brightness, appearing yellowish-white in color, suggesting a significant population of older stars. The outer regions fade gradually into the background, displaying a slightly elongated shape. There is a subtle blueish tint to the very faint outer edges, possibly indicating the presence of a younger, albeit sparse, stellar population. There is no apparent structure, such as spiral arms or a prominent bar. Overall, the galaxy is a relatively undisturbed system, without obvious signs of recent major mergers or tidal interactions.
