This galaxy presents as a system with a relatively smooth, centrally concentrated component, but with clear signs of morphological disturbance. The main body of the galaxy appears mostly featureless, exhibiting a diffuse halo of light. A secondary, distinct component is visible, possibly indicating an ongoing or recent interaction or merger. This secondary component is more compact and presents with a redder hue than the main body. There are hints of tidal features or asymmetries in the outer regions, such as a faint tail or bridge of material. Overall, the galaxy seems to be in a transitional state, having a significant mass, and showing signs of recent or ongoing star formation activity associated with the interacting component. The primary component is somewhat spheroid and appears mostly quiescent.
