The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The color gradient transitions from a bright, yellowish-orange core to fainter, reddish-hued outer regions, indicative of an older stellar population dominating the bulge and a gradual decrease in stellar density towards the galactic edges. No prominent spiral arms or active star-forming regions are readily apparent. Subtle deviations from perfect ellipticity are possibly present, suggesting minor tidal interactions or internal disturbances within the galaxy, though overall the structure appears relatively undisturbed. The galaxy's light profile decreases smoothly from center to edge, consistent with an elliptical galaxy type.
