The galaxy presents as a somewhat smooth, centrally concentrated system. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The galaxy displays an elliptical morphology, with the light distribution tapering off gradually from the core toward the edges. There is a slight suggestion of disk-like structure, although the smoothness predominates, and no distinct spiral arms are discernible in this image. Overall, the galaxy appears relatively undisturbed, showing no strong signs of ongoing mergers or tidal interactions. The colors indicate some ongoing star formation, but not at a prodigious rate.
