The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution and no discernible spiral arm structure. The core is bright and concentrated. It appears slightly elongated. The galaxy appears to be relatively isolated, with a few smaller galaxies nearby that are likely interacting or in the process of merging. Overall, the galaxy appears to be a relatively massive, evolved system, consistent with an elliptical classification. The color suggests an older stellar population.
