The galaxy presents a largely smooth, elliptical morphology. Its light profile is dominated by a concentrated central bulge, showing a gradual decrease in surface brightness with increasing radial distance. There are no easily observable spiral arms. The galaxy is moderately rounded in shape, showing hints of a disk-like structure. There are no distinct tidal tails, bridges or signs of active galactic nuclei, suggesting a quiescent state. The core exhibits a brighter, bluer color, indicative of potential star formation. Overall, the galaxy is not undergoing any significant merging events.