The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its central region exhibits a bright, concentrated core, suggesting a high density of stars. The overall color is yellowish-red, indicative of an older stellar population and a lower rate of ongoing star formation. There is a slight elongation to the galaxy's shape. The lack of obvious spiral arm structures or significant dust lanes further supports its classification as an early-type galaxy. There are no immediately apparent signs of major mergers or tidal disturbances. 
