The galaxy presents as a relatively smooth, elliptical structure. Its core is bright and concentrated, exhibiting a bluish-white hue, suggesting a population of younger, hotter stars in the central region. Moving outwards from the core, the light gradually diffuses, with the outer regions exhibiting a more yellowish tint, possibly indicating an older stellar population. The overall shape is moderately elliptical, not perfectly spherical, nor highly elongated, but somewhere in between the two extremes. There appears to be a lack of significant spiral arm structure or distinct features like dust lanes. The galaxy does not show any strong visual signs of ongoing or recent major merger activity or tidal disturbances; its shape seems largely undisturbed. Overall, this galaxy seems to be a fairly typical example of an elliptical system, potentially in a relatively quiescent state, but additional spectroscopic data would be needed to confirm the age and composition of the stellar populations.
