The galaxy presents as a somewhat rounded, centrally concentrated object. Its morphology appears predominantly smooth, with a fraction exhibiting features suggestive of a disk or disturbances. The light profile diffuses outwards from the center, with no clearly discernible spiral arm structure or bar feature. The overall color is intermediate, showing light in the g, r, and z bands. There is a suggestion of minor asymmetry in the light distribution, potentially indicating a minor interaction or internal disturbance. The galaxy does not exhibit any obvious signs of a major merger, with most suggesting it is undisturbed.
