The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an overall elliptical shape with a hint of a possible disk structure. The central region is dominated by a bright, yellowish-orange light, suggesting an older stellar population. There is a fainter bluish feature on one side, potentially indicating a region of recent star formation. There are some indications of possible minor disturbances or interactions, causing an asymmetry in the galaxy's structure. Overall, this galaxy seems to be a transitioning system, potentially evolving from a more active, star-forming state to a more quiescent one.
