The galaxy appears to be a relatively smooth, elliptical system. It exhibits a spheroidal morphology with no discernible spiral arms or bar structure. The central region is significantly brighter and appears yellowish, suggesting a high concentration of older stars. The light gradually fades toward the outer edges of the galaxy, forming a diffuse halo. There is no evidence of significant dust lanes or active star formation regions within the visible light spectrum. The object appears largely undisturbed, with no apparent signs of tidal interactions or ongoing mergers. It has a roundish shape and shows no indication of any major disturbance.
