This galaxy exhibits a largely spheroidal morphology, characterized by a high degree of central concentration. Its overall color is yellowish, suggesting a stellar population dominated by older, redder stars. The galaxy appears smooth and lacks prominent spiral arm structures or a well-defined disk. There are no obvious signs of recent or ongoing major mergers. The galaxy exhibits a minor degree of asymmetry, but this could be due to its high degree of central concentration. The galaxy's size is moderately extended, but appears consistent with similarly distanced elliptical galaxies.
