The galaxy appears to be a relatively face-on elliptical galaxy, exhibiting a smooth and concentrated morphology. The galaxy shows a centrally bright nucleus which is surrounded by a more diffuse halo. The light profile appears smooth, lacking any distinct spiral arm structures or prominent dust lanes. The overall color suggests a population of older stars, consistent with a low star formation rate. There are potentially some minor disturbances visible, indicating a possibility of a past or ongoing merger event. The galaxy's shape is close to round. The galaxy does not appear to be undergoing a major merging event.
