The galaxy presents a generally smooth and elliptical morphology. There is no clear spiral arm structure visible. The light distribution appears relatively concentrated towards the center, with a gradual decrease in luminosity outwards. The galaxy exhibits a yellowish-orange hue, indicative of an older stellar population. The axial ratio suggests a mostly circular appearance. There is no obvious evidence of a major ongoing merger, but subtle irregularities might indicate minor disturbances. There are no prominent dust lanes or star-forming regions evident in this image.
