The object presents as a galaxy with a smooth, largely featureless morphology. It appears elliptical in shape, exhibiting a high degree of roundness. The galaxy displays a concentrated central bulge that transitions gradually to a more diffuse outer halo. The core region exhibits a yellowish-white hue, potentially indicating an older stellar population. Moving outwards, the halo appears slightly bluer, suggesting the presence of younger stars, although this is not highly pronounced. There is no visible evidence of spiral arms, a bar, or significant dust lanes. No signs of tidal distortions or ongoing mergers are readily apparent in the image. The galaxy appears to be relatively isolated, without obvious nearby interacting companions. The overall color suggests an intermediate redshift object. The relative smoothness and lack of distinct features indicates a relatively evolved system. The weak blue coloration indicates the presence of some ongoing star formation within the galaxy.
