The galaxy presents as a largely featureless, smooth elliptical galaxy. The light profile appears centrally concentrated with a gradual decrease in intensity towards the outer regions. The core exhibits a slightly reddish hue, possibly indicative of an older stellar population. Fainter, greenish extended emission surrounds the redder core, which may hint at a small amount of ongoing star formation. There is no clear evidence of spiral arms, a prominent disk, or major disturbances due to interactions or mergers. The overall shape is close to circular, suggesting minimal ellipticity.
