The galaxy appears as a somewhat elongated, elliptical structure, presenting a smooth, largely featureless profile in this image. The galaxy exhibits a radial color gradient, transitioning from a yellowish-white core to slightly bluer hues in the outer regions. The core appears to be dominated by an older stellar population, as indicated by its yellow color. The outer regions hint at the presence of some younger, bluer stars, albeit at a low star formation rate. The overall structure suggests minimal tidal disruption or ongoing merger activity. The morphology indicates it is likely an elliptical galaxy, potentially exhibiting a slight disk-like component.
