The galaxy presents as a primarily elliptical or lenticular structure, exhibiting a smooth, concentrated light profile. There is minimal evidence of spiral arms or significant dust lanes. The galaxy appears to be relatively round, with only a slight deviation from circular symmetry.  The color appears somewhat redder suggesting an older stellar population. The galaxy exhibits a central bulge with a more diffuse halo. The system does not appear to be undergoing any major merging events or strong tidal interactions, and shows a relatively undisturbed structure. Overall, the galaxy appears to be a relatively quiescent system with a substantial mass and a low rate of star formation.
