This galaxy presents as a smooth, elongated structure, consistent with a likely elliptical morphology. The central region exhibits a higher concentration of light, gradually decreasing in intensity towards the outer edges. The color gradient suggests a dominance of older stellar populations, with a yellowish-orange hue indicative of a relatively low rate of ongoing star formation. The galaxy shows no apparent spiral arms or significant dust lanes. There is a hint of tidal disturbance, with a very minor irregularity to the shape. The galaxy displays a small angular size, suggesting a considerable distance. It appears to be a relatively massive system, based on its overall brightness and smooth morphology. The high degree of smoothness suggests that it is fairly relaxed and well evolved.
