The galaxy presents a roughly elliptical morphology, appearing largely smooth in structure. The central bulge exhibits a bright, yellowish-white color, suggesting an older stellar population. Extending outward from the bulge, a fainter, bluer halo is observed, which may indicate the presence of some younger stars. Possible features include a slight distortion in the galaxy's overall shape, suggestive of a minor gravitational disturbance. The object appears to be a massive galaxy with a moderate rate of star formation. A weak disk structure may be present. There is a hint of a potential merging event in its past.