The galaxy presents a somewhat elliptical morphology, exhibiting a smooth, concentrated central bulge that appears to dominate its overall structure. The light distribution suggests a high degree of radial concentration toward the core. There is faint indication of a possible disk component that isn't especially distinct. There are suggestions of minor disturbances in the form of faint, irregular extensions or asymmetries in the outer regions of the disk. These disturbances could be indicative of tidal interactions or recent minor mergers. The galaxy is intermediate in roundness. The galaxy appears to have very low rate of star formation activity. The general color of the galaxy indicates a relatively evolved stellar population.
