The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. It exhibits a generally round shape with some slight deviation. Its light is dominated by yellow hues, suggestive of an older stellar population with relatively suppressed recent star formation. There is minimal evidence of any distinct spiral arm structure or prominent dust lanes; the disk structure is suppressed. There appear to be no major distortions or tidal features indicative of recent major mergers. The overall appearance suggests a system nearing quiescence.