The galaxy presents a generally smooth morphology. It appears elliptical, with a high degree of circularity. The central region is characterized by a concentrated, bright yellowish-white core, suggesting a significant population of older stars. This central bulge gradually diffuses outwards, fading into a less luminous, more extended halo. There is no visible spiral arm structure, nor any indication of significant dust lanes or ongoing major merging activity. The galaxy seems to be relatively undisturbed. There is a subtle color gradient from the center outwards.
