This galaxy presents as an elongated, somewhat disturbed system. The core exhibits a bright, concentrated luminosity, suggesting a significant density of stars and possibly an active galactic nucleus. Moving outwards from the core, there appears to be a gradual decrease in luminosity. A hint of spiral structure or tidal arms can be seen extending from the central region, but the features appear disrupted and irregular. The overall color gradient shifts from yellowish-white in the center to a bluer tint in the outer regions, which could suggest younger stellar populations present in the outer parts of the galaxy. The galaxy shows signs of a potential past or ongoing merger event, indicated by the asymmetries and the disturbed morphology. There might be ongoing star formation, concentrated in localized areas away from the core. Overall, it seems to be a sizable galaxy with some notable internal activity.
