The galaxy presents as a relatively smooth, centrally concentrated object with a largely elliptical morphology. It exhibits a yellowish hue indicative of an older stellar population, suggesting that star formation is likely not occurring at a high rate within the galaxy at the current epoch. There's no significant dust lane or arm structure apparent, lending further credence to a lack of ongoing significant star formation. Overall, the galaxy appears to be a spheroidal system that has undergone significant evolution. There are no major signs of disturbances or mergers, hinting at a dynamically relaxed system.
