The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, fading gradually towards the outer edges. There is a slight asymmetry in the outer isophotes, which could be due to a minor gravitational interaction or disturbance. The core appears bright and unresolved. The color is relatively uniform across the galaxy, with a redder hue suggesting an older stellar population. There is no strong evidence of spiral arm structure or significant dust lanes. The overall appearance is consistent with an elliptical galaxy type.
