The galaxy presents as a relatively smooth, lenticular or early-type spiral system. There's a bright, concentrated central bulge that dominates the overall appearance. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. The disk is faint and indistinct, appearing more elliptical than circular, with only very subtle suggestions of spiral arm structures. There is a small amount of bluer light in the outer regions of the galaxy, but is not indicative of active star formation. The lack of strong features and the dominant bulge suggest a system that has largely ceased active star formation, with a stellar mass slightly below the median for galaxies. No significant tidal features or signs of recent mergers are apparent. The galaxy appears stable and relatively undisturbed.
