The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is yellowish-white in color, which gradually fades into a fainter, more diffuse halo. The galaxy displays a high degree of radial symmetry, appearing almost perfectly round. There is a very slight suggestion of tidal features or minor disturbances. The color profile indicates an older stellar population, with a significant lack of blue star-forming regions typically associated with spiral arms. Overall, the object appears to be a mature, passively evolving galaxy, with negligible recent star formation activity.
