This galaxy exhibits an overall elliptical morphology. A bright, concentrated central bulge dominates the luminosity profile, indicating a likely high stellar density in this region. The bulge appears to be primarily composed of older stellar populations, implied by its yellowish-orange color. Fainter, less concentrated light extends outwards from the bulge, forming a diffuse halo. There is only a hint of bluer light towards the edges of the galaxy. There are no apparent signs of spiral arms or strong tidal disturbances. The galaxy appears relatively undisturbed.
