The galaxy presents a generally smooth, elliptical morphology. It appears to be relatively undisturbed, showing minimal signs of ongoing or recent mergers. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges. The galaxy's color suggests a lack of significant ongoing star formation, with a redder hue indicating an older stellar population. The overall structure appears quite compact, presenting a shape close to spherical. There is a very faint disk like structure but it is hard to determine due to the angle and lack of star formation.
