The galaxy presents as a somewhat concentrated, yet diffuse, central region with extended, fainter arms or features. The core exhibits a yellowish-orange hue, suggestive of an older stellar population and potentially lower star formation rates. The outer regions appear more irregular, with bluer tinges hinting at the presence of younger, hotter stars and ongoing star formation activity. Some distortions and features suggest a possible past interaction or merger event, with a few clumps of luminous matter scattered irregularly throughout the structure. The overall impression is of a galaxy that is likely evolved but not entirely quiescent.
