The galaxy presents as an elliptical morphology, appearing largely smooth with a concentrated central bulge. The light profile decreases gradually from the core outwards, lacking distinct spiral arm structures. The overall color is yellowish-white, suggesting an older stellar population with a lower rate of on-going star formation, based on the lack of prominent blue hues typically associated with young, massive stars. It is elongated, but not highly so, with a ratio of major to minor axis that suggests it is neither perfectly spherical nor highly flattened. There are subtle indications of some tidal features, perhaps minor disturbances indicating past or ongoing interactions with smaller companions. The galaxy appears relatively isolated, not exhibiting obvious signs of a major merger event in progress, although some level of past interaction cannot be ruled out.
