The galaxy presents as a somewhat elongated, elliptical-like structure. It exhibits a smooth, featureless appearance without discernible spiral arms or a prominent disk. The light distribution indicates a concentration of older stars toward the center, giving a yellowish-orange hue which fades gradually into green around its halo. A slight asymmetry is noticeable, suggesting a minor disturbance or interaction in its past, potentially a small merger. Overall, the galaxy appears to be a relatively evolved system, with indications of ongoing star formation activity, albeit at a moderate level. The object is likely quite massive.
