The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape appears approximately elliptical, exhibiting a high degree of roundness with minimal elongation. A distinct central bulge is visible, characterized by a bright, concentrated luminosity profile suggesting a high stellar density. The outer regions of the galaxy display a gradual fading of light intensity, indicating a diffuse stellar halo. Faint bluish regions are observed within the galaxy, potentially indicative of ongoing star formation. There is a slight suggestion of minor disturbances or asymmetries in the outer regions, but no prominent tidal features or signs of a major ongoing merger are immediately apparent.
