The galaxy presents an overall elliptical morphology, displaying a smooth and concentrated light profile. The central region exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outwards from the core, the galaxy's color appears to shift slightly toward a redder tone, suggesting a possible gradient in stellar age and/or metallicity. There is subtle evidence of a faint, extended halo surrounding the main body of the galaxy. No prominent spiral arms or significant dust lanes are discernible. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. 
