The galaxy appears to be a luminous, centrally concentrated object with a yellowish-white core region. The morphology suggests a possible classification as an elliptical or lenticular galaxy due to its relatively smooth appearance and lack of distinct spiral arm structures. The shape is close to round, with a slight elongation. There is a hint of a disk-like structure, or disturbed features present in the galaxy, which is a more diffuse region surrounding the core. Evidence is present of merging occurring within the system. This is observed by multiple asymmetric features, with a prominent disturbance or possible tidal tail extending away from the main body. The overall color of the galaxy suggests a stellar population dominated by older stars.
