The galaxy presents a largely smooth, elliptical morphology, appearing somewhat rounded in shape. Its color gradient indicates an older stellar population, concentrated primarily within the central bulge. The bulge exhibits a strong yellow to orange hue, suggesting evolved stars with lower rates of star formation. A faint, bluish region is seen on one edge of the galaxy, hinting at a minor disturbance, possibly indicative of tidal interactions. This region may host pockets of younger, hotter stars, albeit less prominent than the older population. Overall, the galaxy appears relatively undisturbed with only slight visual indications of past or ongoing interactions. The light distribution suggests a high degree of symmetry, consistent with an elliptical galaxy.
