This galaxy exhibits a generally smooth, elliptical morphology. The light is concentrated towards the core, which displays a yellowish-orange hue, indicative of an older stellar population. The galaxy appears somewhat elongated rather than perfectly spherical, exhibiting a moderate ellipticity. There is no apparent dust lane or spiral arm structure visible. The outer regions fade into the background sky without any distinct, sharp edges. There is no indication of ongoing major mergers, though there appears to be some minor irregularity in the surrounding halo.
