The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-white hue at its core, indicative of an older stellar population. The outer regions display a gradual fading in intensity, with hints of reddish tones, possibly due to dust or a population of cooler, older stars. There is a subtle suggestion of a disk-like component, although it is not distinctly defined, leading to an overall classification favoring a smooth morphology. Minor irregularities or disturbances are potentially present in the form of subtle extensions or asymmetries, suggesting a possible past or ongoing interaction, but are not particularly prominent. The galaxy shows no readily observable signs of active star formation.
