The galaxy presents an elliptical morphology, with a high degree of central concentration. It appears relatively smooth in structure. The core exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, there is a noticeable decrease in luminosity and a subtle transition towards a bluish-green tinge in the outer regions. There is no readily apparent spiral arm structure, barring the suggestion of a very faint, disturbed, or diffuse disk with a relatively low star formation rate. The galaxy shows an absence of significant dust lanes or prominent star-forming regions. It does not show any signs of a recent major merger event. The overall shape is moderately elongated, closer to ellipsoidal than spherical, with an intermediate axis ratio.
