The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. It appears largely spheroidal in shape, exhibiting minimal disk structure. The light distribution is quite uniform, with a gradual decrease in intensity from the center outwards. There are some indications of minor disturbances in the morphology. It seems the galaxy might be in the process of merging with other galaxies. The color index suggests an older stellar population, which is consistent with its smooth morphology and presumed high mass. The subdued blue light indicates a relatively low star formation rate.
