The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that appears near-spherical. The light profile appears to fade gradually from the center outward, lacking prominent spiral arm structures or distinct features. There's a slight color gradient visible, with the central region displaying a yellow to gold hue, potentially indicative of an older stellar population. Fainter, bluer light is observed in the outer regions, suggesting the presence of some younger, hotter stars, though this is not substantial. There's no evidence of significant ongoing mergers or tidal disturbances in this image, and it is not clear if this galaxy is interacting with neighboring systems.
