The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The color profile suggests an older stellar population dominating the light output, particularly in the central regions, which exhibit a yellowish-orange hue. The outer regions appear somewhat bluer, hinting at the presence of younger stars or a small amount of ongoing star formation, though it is not the dominant process. There may be some subtle indication of minor tidal disturbance or interaction occurring, potentially a faint plume or asymmetry. Overall, the galaxy is a massive system.
