The galaxy appears as a somewhat elongated spheroid, exhibiting a smooth, diffuse light distribution. The primary color is a yellowish-white, suggesting an older stellar population. The galaxy displays a slight asymmetry in its profile, leaning toward an elliptical shape. The color and lack of discernible substructure indicate minimal ongoing star formation. There is a faint hint of blue at the edges which may indicate the presence of younger, hotter stars on the edge of the galaxy. Overall, the galaxy appears to be a relatively massive system, likely with a considerable bulge component. There is a slight indication of tidal disruption occurring within the galaxy.
