The galaxy presents a relatively smooth and centrally concentrated morphology. The object is elliptical in shape. Its color profile suggests a population of older stars, indicated by the reddish-yellow hue. There may be very faint and subtle asymmetric extensions present but this requires further investigation. There is no clear evidence of spiral arm structure. The object seems undisturbed, with no indications of a recent major merger event. Star formation appears suppressed within the galaxy.
