The object presents as a centrally concentrated galaxy with a smooth light distribution.  It appears largely spheroidal in shape, exhibiting a high degree of circular symmetry, with only a slight deviation towards ellipticity. The galaxy's color is generally consistent with an older stellar population, though some bluer regions are present closer to the center of the galaxy. There are hints of some minor disturbances present in the image. These seem to be primarily close to the galaxy center, and may be the result of smaller galactic objects merging. Based on the color and smooth profile, the galaxy is likely an elliptical or S0 type.
