The galaxy presents a generally smooth morphology, appearing elliptical in shape. The central region exhibits a high concentration of light, indicating a prominent galactic bulge. The outer regions gradually fade, lacking distinct spiral arm structures. The galaxy's color profile suggests a population of older stars, with a subtle blue tint in the outer edges possibly indicating some ongoing, but limited, star formation. There may be a minor gravitational disturbance and possible faint merger visible within the galactic halo.
