The galaxy appears as a slightly elongated spheroid, suggesting an elliptical morphology, although subtle disk-like features cannot be entirely ruled out. The light distribution appears relatively smooth and centrally concentrated, with no immediately obvious spiral arm structures or prominent dust lanes. There's a general even color gradient. The relative lack of irregular features indicates that the galaxy is likely not undergoing a major merging event. The overall color suggests that the stellar population is a mix of old and young stars. Star formation is present but at a low rate.
