The galaxy presents a smooth, elliptical morphology, displaying a concentrated central bulge that graduates outward into a more diffuse halo. The overall color profile suggests an older stellar population, with a yellowish hue indicative of a dearth of ongoing, high-mass star formation. There's little evidence of prominent spiral arms or distinct disk features, supporting the smooth classification. The morphology appears undisturbed, with no significant tidal features or morphological irregularities that would suggest a recent major merger event, though a slight asymmetry suggests a minor disturbance. The roundness of the galaxy suggests it is not viewed edge-on.
