The galaxy presents as a single, relatively smooth object with a concentrated central region. Its morphology is generally elliptical, appearing more elongated than perfectly circular. The color profile exhibits a dominant yellowish-orange hue, suggesting an older stellar population. A faint greenish tint is visible in the outer regions, but this may be due to image artifacts. There is no discernible spiral structure or significant dust lane obscuration evident. No tidal tails or other clear signs of recent major merger events are present, although the outer edges are not sharply defined. This could indicate a slight gravitational interaction or past minor merger event.
