The galaxy presents as a generally smooth, elliptical structure with a noticeable concentration of light towards its center. The core region appears to be quite dense, exhibiting a bright, relatively uniform glow. Moving outward from the center, the light gradually diffuses, suggesting a decreasing stellar density with increasing radius. The overall color profile is slightly reddish, hinting at an older stellar population and reduced ongoing star formation. There is subtle evidence of some minor asymmetry in the outer regions, possibly indicative of past interactions or disturbances, but no clear spiral arm structures or distinct features are visible. The galaxy appears relatively isolated with no major nearby companions or signs of a recent major merger.
