The galaxy presents as a slightly elongated, lenticular-like structure. The central region exhibits a high surface brightness, appearing almost stellar in its intensity. The color of the central region is bluish-white, suggestive of a population of hot, young stars or a potential active galactic nucleus. A subtle color gradient is observed moving outward from the center. The outer regions become progressively fainter and redder, indicating an aging stellar population with fewer ongoing star formation events. The galaxy's shape is somewhat flattened. There is no clear evidence of spiral arms or a distinct disk, leading to the classification as lenticular. Overall, the galaxy appears to be a relatively evolved system, with a dominant bulge and a fading disk.
