The galaxy presents as a somewhat flattened elliptical or lenticular type system. It appears largely featureless with a smooth, diffuse light distribution. The central region displays a slight concentration of luminosity suggesting a small galactic bulge. There is a very subtle color gradient, appearing bluer towards the outer regions. The galaxy shows minimal evidence of spiral arm structure or significant dust lanes, indicative of a relatively quiescent system with little active star formation. The overall morphology suggests a galaxy that has likely undergone significant evolutionary processes, potentially including mergers or interactions, resulting in the smooth, featureless appearance and the suppression of star formation.
