The galaxy presents as a largely spheroidal object. It exhibits a smooth, seemingly undisturbed morphology with a high degree of central concentration. The color profile suggests an older stellar population, with a dominant yellow hue. There is no apparent structure such as spiral arms or a prominent disk component visible at this resolution. The overall shape appears quite round, with only a subtle deviation toward elongation. Visual inspection does not reveal any indications of ongoing major merger activity or significant tidal disturbances, however there is a possibility of minor disturbance. Based on the color and morphology, this is likely an elliptical galaxy with a relatively low star formation rate.
