The galaxy appears as a centrally concentrated object with a smooth overall morphology. It exhibits an elliptical or lenticular form, lacking prominent spiral arms. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, potentially indicative of a bulge composed of evolved stars. There is a slight hint of bluer light in the outer regions, suggestive of some ongoing, though potentially low level, star formation. The galaxy appears relatively undisturbed, exhibiting no significant signs of tidal interactions or major merger events. Its shape appears to be closer to an elliptical galaxy than a spiral.
