The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated, diminishing gradually outward. There is a notable lack of distinct spiral arms or prominent dust lanes. The color is generally yellow-white, indicating a stellar population dominated by older, less massive stars with relatively low ongoing star formation. The galaxy exhibits a high degree of roundness in its shape. There is no strong evidence of tidal distortions or ongoing major merging events. The galaxy's size appears relatively compact.
