The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits an overall elliptical morphology, appearing somewhat rounded rather than highly elongated. The core is a bright, intensely luminous region that dominates the galaxy's visual appearance. Moving outward from the core, the light gradually fades into a diffuse halo. There is minimal evidence of spiral arms or significant dust lanes. Subtle color gradients are observed, with the central bulge exhibiting a slightly more yellow-orange hue, potentially indicative of an older stellar population. The outer regions appear somewhat bluer, suggesting the presence of younger stars, though overall star formation appears low. There is no visually obvious evidence of recent mergers or major tidal disturbances. Faint, very subtle features may exist in the outer halo, but resolution is limited. The galaxy is a massive system with high luminosity.