The galaxy presents a generally smooth, elliptical morphology, suggesting an older stellar population. The central region exhibits a high concentration of luminosity, appearing nearly spheroidal and indicative of a significant bulge component. A slight elongation is observed, hinting at a shape that deviates somewhat from perfect circularity, possibly closer to an in between shape. There appears to be a slight asymmetry or minor perturbation in the galactic structure, as indicated by a subtle distortion in the outer regions, but no major disturbances. The overall color suggests a moderate amount of star formation, though the dominant hue points to evolved stars.
