The galaxy presents as a somewhat smooth, elliptical-like structure with a concentrated central bulge that appears bright, potentially indicating a high density of stars or an active galactic nucleus. There's a gradual decrease in luminosity from the center outwards. A faint disk like structure is visible around the central bulge. The galaxy shows no obvious signs of major disturbances, such as tidal tails or strong asymmetries, but subtle distortions are present indicating possibly a minor merger. The galaxy has a slight blue tint, which suggests the presence of younger, hotter stars. Overall, the galaxy appears to be in an intermediate stage of evolution, possibly transitioning from a more actively star-forming system to a more quiescent one.
