The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated toward the center, with a gradual decrease in brightness outward, extending to a radial distance of approximately 10 kpc. There is a slight elongation in its overall shape, but it appears largely spheroidal. The galaxy exhibits a yellowish-orange color, suggesting a population of older stars and a lack of significant ongoing star formation. The overall structure indicates the possibility of a relaxed system, with no major mergers or disturbances readily apparent, although there may be evidence of minor tidal interactions or past mergers present in the outer regions.
