The galaxy presents a generally smooth, elliptical morphology. It exhibits a central, concentrated bulge region that appears yellowish-orange in color, suggesting an older stellar population. The outer regions of the galaxy are more diffuse and display a slightly bluer tint, which could be indicative of a younger stellar population or ongoing star formation. There are no prominent spiral arms or bar structures visible. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger. A slight elongation is observable, but the overall shape approximates a rounded form. The color gradient from the center to the outer edges may imply a radial variation in stellar population ages or dust content.
