The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a bright, concentrated luminosity that diminishes gradually towards the outer regions, lacking distinct spiral arm features. The ellipticity appears slight, trending toward a nearly circular form. No apparent signs of major mergers or significant tidal disturbances are visually detected. The light distribution suggests a centrally concentrated spheroid, consistent with an older stellar population. Faint reddish tones are observed in the outer regions.