The galaxy presents a generally smooth appearance. The central bulge is a bright, concentrated region, appearing almost circular. Surrounding the bulge, a more diffuse region of light extends outward, exhibiting a slightly elongated or elliptical shape. This outer region seems less structured than a spiral galaxy, but not perfectly spherical. There may be a subtle hint of a disk-like component or a faint feature. The overall color is a blend, with the central bulge appearing more yellow/white, potentially indicating an older stellar population. The outer regions show a faint bluish tint suggesting the presence of younger, hotter stars. There is a suggestion of a possible minor disturbance in the galaxy's shape, although definitive signs of a merger are not clearly visible. The main body of the galaxy is fairly compact, with no obviously extended tidal tails or strong distortions. 
