The galaxy appears as a largely featureless, elliptical-like object. It exhibits a concentrated central bulge with a diffuse, extended halo. The color gradient suggests an older stellar population, with a yellowish-white core and a slightly bluer outer region. There's no clear evidence of spiral arms or active star formation regions. The galaxy is generally smooth in appearance, showing high degree of rotational symmetry. It does not show signs of any recent or ongoing major mergers. Small disturbances can not be ruled out.
