The galaxy presents a compact, elliptical morphology. Its light profile is smooth and concentrated towards the center, displaying a lack of defined spiral arms or a prominent disk structure. There is a subtle elongation in its overall shape. The color of the galaxy appears to be predominantly redder, suggesting an older stellar population and relatively low ongoing star formation activity. There are some indications of minor disturbances, likely from small tidal interactions. The galaxy exhibits properties consistent with a significant mass.
