The galaxy presents as a centrally concentrated, somewhat elliptical structure. The core region exhibits a high surface brightness, appearing nearly spherical and yellow in color, suggesting an older stellar population. Moving outward from the core, the surface brightness decreases, with the outer regions appearing more diffuse and subtly elongated. There is a hint of a disk-like structure, but any spiral arm features are not clearly resolved. There are no obvious signs of any major tidal disturbances or recent merger activity. The galaxy appears relatively undisturbed and well-defined.
