The galaxy presents as a relatively smooth, elliptical structure. Its overall color profile suggests a population of older stars, with a dominant yellowish hue. There is a slight elongation in its shape, indicating it is more cigar-shaped than completely spherical. There is no apparent evidence of active galactic nuclei or significant star formation. The galaxy appears undisturbed, with no obvious signs of mergers or tidal interactions. Its structure appears relatively homogenous, lacking distinct features such as spiral arms or a prominent central bar. The galaxy's estimated mass range is on the higher side, and its rate of star formation is estimated to be slow.
