The galaxy presents as a relatively smooth, yet somewhat disturbed structure, with what appear to be significant tidal features suggesting an ongoing or recent merger event. The primary body of the galaxy exhibits an overall elliptical morphology, with the majority of light concentrated towards the center, indicating a developed stellar population. A small amount of irregular distribution of bluer light towards the outskirts suggests ongoing, although likely subdued, star formation in certain regions. Based on the faint tidal structures, there appears to be a secondary galaxy merging with it. Overall, the system is complex and likely in the intermediate stages of a major merger, where dynamical relaxation is not yet complete.
