The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a bright central bulge which gradually fades into a more diffuse halo. There is a suggestion of a disk component although no spiral arm structure is visible. The galaxy appears elongated, with a ratio of major to minor axes suggesting it is not perfectly spherical. There may be evidence of a minor tidal disturbance in the outer regions of the galaxy, possibly due to an interaction. The light profile of the galaxy shifts from bluer in the outer disk to redder in the central bulge. Based on the redder color profile of the galaxy, star formation is not particularly active.
