The galaxy appears as an elliptical or lenticular type galaxy, based on its smooth and rounded morphology. The galaxy's light profile suggests a dominant bulge, exhibiting a high degree of central concentration. There is little evidence of a disk-like structure or spiral arms, and no significant dust lanes are visible. The color is generally yellowish suggesting an older stellar population, with a minimal amount of young, blue stars. There are no obvious signs of tidal disturbances or ongoing major mergers with other galaxies, although the galaxy may have undergone minor interactions with other galaxies. The apparent size is relatively compact, with a high degree of symmetry.
