This galaxy presents as an elliptical, relatively smooth object with a moderate axial ratio. The core appears quite concentrated, displaying a yellowish hue which may indicate a significant population of older stars.  Faint, diffuse outer regions are visible, extending along the major axis. These regions exhibit a slightly bluer color compared to the core, possibly indicating more recent, though subdued, star formation. There are no apparent signs of active galactic nuclei activity, nor is there any obvious spiral structure or substantial dust lane obscuration. No major mergers or tidal disturbances are obvious upon visual inspection. However, there are some hints of minor disturbances that may indicate a past interaction with another galaxy.
