This galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. The overall shape is slightly elongated but generally round. There is no clear evidence of spiral arm structure or a prominent disk. The color is predominantly yellow/orange, suggesting an older stellar population with relatively low levels of ongoing star formation. There are no obvious signs of major tidal disturbances or ongoing mergers, though minor disturbances are possible. The galaxy is relatively massive, as indicated by its absolute magnitude.
