The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round, though with a slight deviation. The galaxy's core is bright and dominant, indicative of a high concentration of stars. There is a subtle color gradient visible, with the central region appearing bluer than the outer regions, suggesting younger stellar populations in the core. The outer regions of the galaxy are less defined and appear redder. No prominent spiral arms or a distinct disk structure are observable. There are subtle hints of minor disturbances or faint tidal features. The galaxy does not appear to be undergoing a major merger or experiencing significant tidal interactions.
