The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elongated morphology, appearing somewhat in between round and elliptical. The light distribution appears largely uniform across the galaxy, with a gentle falloff in intensity towards the outer edges. There is a subtle hint of a possible disk or some internal structure, but it is not strongly pronounced. No major disturbances or signs of merging are readily apparent, although a very minor tidal interaction cannot be ruled out due to a subtle asymmetry in the outer isophotes. Overall, the galaxy appears to be a fairly evolved system, with the bulk of its stellar population likely being older. The galaxy is moderately luminous.
