The galaxy appears as a centrally concentrated, elliptical-like system with a smooth light distribution. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy appears nearly round in shape. I do not observe any major disturbances in its morphology, suggesting a lack of recent major merger activity. The color of the galaxy is slightly on the redder side, indicating an older stellar population, though some blue light is present. There is some evidence of minor disturbance, perhaps indicating low-level ongoing interactions or past minor merger events.
