The galaxy presents a generally smooth and rounded morphology. It appears as a single, concentrated object with a bright, yellowish core that gradually fades outwards to a more diffuse halo. There are no apparent spiral arms or significant dust lanes visible, suggesting an elliptical or lenticular type galaxy. Minor disturbances may be present in the outer regions, but the galaxy does not appear to be undergoing a major merger or strong tidal interaction. Its color profile suggests a population of older stars, with relatively low levels of ongoing star formation.
