The galaxy appears as a relatively compact and luminous object. It exhibits a smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The light is concentrated towards the center, suggesting a high degree of central mass concentration. The galaxy appears to have undergone, or may be undergoing, a merger event based on visual features. There are no prominent tidal tails and no other signs of recent interactions. The dominant color is reddish, indicating a stellar population dominated by older stars. The small amount of blue light could be indicative of ongoing, though perhaps limited, star formation.
