The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, indicated by the brighter, yellowish hue, which gradually diffuses outward. The overall shape appears largely undisturbed, with no obvious signs of tidal tails or major mergers. A subtle disk structure may be present. The galaxy is relatively massive. Based on the color indices, the galaxy appears to be composed primarily of older stellar populations, suggesting a suppressed rate of star formation. 
