The galaxy presents a smooth, elliptical morphology. It appears relatively round, exhibiting only a slight deviation from perfect circularity. The color profile suggests a concentration of older stellar populations, with a predominantly yellow hue. There is no evidence of spiral arms, a central bar, or significant dust lanes. The galaxy appears to be relatively isolated, showing no signs of major interaction or ongoing merger activity. The smooth light distribution and color indicate that star formation activity is likely low.
