The galaxy appears to be a relatively smooth, centrally concentrated object. It presents an elliptical morphology, exhibiting a somewhat spheroidal shape rather than a distinct disk-like structure. Coloration suggests a dominance of older stellar populations, with a yellowish hue indicative of a dearth of ongoing star formation. There are no prominent spiral arms or dust lanes visible. The galaxy exhibits a slight asymmetry, but no obvious signs of a major merger event are observed, although some minor disturbance to the galaxy's structure may be present. The concentration of light towards the center suggests a substantial central bulge. The angular size of the galaxy is relatively compact.
