The galaxy presents as a luminous, centrally concentrated system. Its overall morphology appears relatively smooth, with a high degree of central concentration indicating an elliptical or lenticular classification. The light profile suggests a dominant bulge component. The isophotes are generally round. There is little to no evidence of spiral arm structure or significant dust lanes, indicative of minimal recent star formation activity. The color is yellowish, consistent with an older stellar population. There are no signs of tidal features, strong gravitational lensing effects, or active galactic nucleus activity discernible in this image. The system appears to be a relatively undisturbed galaxy.
