The galaxy presents as a relatively smooth elliptical structure with a bright, concentrated core region exhibiting a yellowish hue. A fainter, more diffuse halo surrounds the core, displaying a bluish tint. The overall shape is elongated, with the major axis oriented approximately northeast to southwest. There is no discernible spiral arm structure or dust lane features visible. The light distribution appears to follow a gradual decline from the core outward, suggesting a relatively old stellar population within the galaxy. Subtle variations in color and intensity within the halo may indicate regions of differing stellar densities or compositions, but high resolution imaging is necessary for further analysis. The system appears undisturbed, with no apparent signs of recent mergers or tidal interactions.
