The galaxy presents a diffuse, yellowish-orange hue, suggesting a dominant population of older stars. The morphological classification appears to lean towards a smooth structure, with a possible spheroidal or elliptical shape. There may be some irregularities or disturbances present. A faint reddish region is present toward the bottom of the galaxy's halo. Overall, this galaxy has an estimated high mass, but fairly little star formation. The galaxy may be in the process of merging.
