The galaxy presents as a centrally concentrated object with a smooth morphology. The core region exhibits a high degree of brightness, suggesting a significant concentration of stars or an active galactic nucleus. The overall shape appears elliptical, though some irregularities are present in the outer regions. There may be some minor tidal disturbances or faint features suggestive of a past minor merger event, specifically in the halo. Color gradients indicate a potential variation in stellar populations, with the central region exhibiting a bluer hue compared to the outer halo. The halo also has a redder tint than the center of the galaxy. Overall the galaxy has a smooth appearance. 
