The galaxy presents as a single, concentrated body with a smooth, elliptical morphology. A distinct central bulge is observed, characterized by a bright, yellowish hue, suggesting an older stellar population. The outer regions of the galaxy gradually fade in intensity, displaying a more diffuse and reddish tint. No spiral arm structures or significant dust lanes are discernible within the observed light. There are no apparent signs of tidal interactions or recent merger events, the overall impression is one of a relatively undisturbed, evolved system.
