The galaxy presents as a system exhibiting interacting components. The primary structure appears elliptical with a relatively smooth texture. This central object displays a concentration of older stellar populations, indicated by its yellowish-orange hue. 

A distinct blue region lies adjacent to the brighter yellowish center, which suggests ongoing star formation activity. This region indicates the presence of younger, hotter stars. 

There appears to be some disruption to the overall symmetry of the main galaxy, possibly due to tidal interactions or minor mergers. A faint extension or tidal tail is observed. Overall, the system appears to be in the intermediate stages of a merger, displaying characteristics of both smooth morphology and ongoing star formation.
