The galaxy appears as a fairly smooth, elliptical-like structure with a concentrated, bright core. Its color profile suggests a relatively older stellar population, leaning towards a redder hue throughout the galaxy, particularly in the central region. There is minimal visible dust or distinct spiral arm structure. The overall shape seems quite regular and symmetrical. The galaxy lacks any obvious signs of ongoing major mergers or significant tidal disturbances. Faint extensions of light surrounding the main body suggest a diffuse halo, though detailed structure within this halo is not apparent.
