The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, concentrated morphology. It displays a fairly regular shape with no obvious spiral arm structure or significant dust lanes. The central bulge is prominent and relatively bright, showing a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy fade in brightness, suggesting a decrease in stellar density with increasing radius. There are no apparent signs of major tidal disturbances or ongoing mergers, however, minor disturbances are not excluded.
