The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests an older stellar population, evidenced by the dominant yellowish-orange hue, indicative of evolved stars and a reduced rate of ongoing star formation. The axial ratio indicates a slightly elongated shape, deviating moderately from a perfect sphere. There is a suggestion of minor disturbance, possibly interaction, as indicated by a slight irregularity in the outer isophotes, but no major merging events are apparent. The overall appearance is consistent with a galaxy transitioning towards a passive, quiescent state.
