The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated, yellowish-orange hue suggesting an older stellar population. The light then transitions to a more diffuse, pale-blue halo extending outwards, potentially indicative of more recent, albeit limited, star formation activity. The overall shape appears slightly elongated rather than perfectly spherical. There is some subtle evidence of possible minor tidal disturbances in the outer regions, but not significant enough to classify it as a major merger.
