The galaxy presents as a centrally concentrated, smooth structure with a largely elliptical morphology. A bright, yellowish core dominates the image, suggesting an older stellar population. The radial color profile appears to redden towards the center. Little to no visible substructure, such as spiral arms or dust lanes, can be discerned. The galaxy appears relatively isolated, lacking obvious signs of tidal interaction or recent merger activity. The overall impression is that of a mature, passively evolving system.
